A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei
by
, , , , , , , , , , , , and
Luigi Foschini
1,*,
Matthew L. Lister
2,
Heinz Andernach
3,
Stefano Ciroi
4,
Paola Marziani
5
,
Sonia Antón
6,
Marco Berton
7,
Elena Dalla Bontà
4,
Emilia Järvelä
8,
Maria J. M. Marchã
9,
Patrizia Romano
1,
Merja Tornikoski
10,
Stefano Vercellone
1 and
Amelia Vietri
4 1
Osservatorio Astronomico di Brera, Istituto Nazionale di Astrofisica (INAF), 23807 Merate, Italy
2
Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA
3
Departamento de Astronomía, Universidad Guanajuato, Callejón de Jalisco s/n, Guanajuato 36023, Mexico
4
Dipartimento di Fisica e Astronomia, Università di Padova, 35122 Padova, Italy
5
Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica (INAF), 35122 Padova, Italy
6
Centro de Física da UC, Departamento de Física, Universidade de Coimbra, 3004-516 Coimbra, Portugal
7
European Southern Observatory (ESO), Santiago de Chile 19001, Chile
8
European Space Astronomy Centre (ESAC), European Space Agency (ESA), 28692 Villanueva de la Cañada, Spain
9
Physics and Astronomy Department, University College London, London WC1E 6BT, UK
10
Metsähovi Radio Observatory, Aalto University, 02540 Kylmälä, Finland
*
Author to whom correspondence should be addressed.
Universe 2022, 8(11), 587; https://doi.org/10.3390/universe8110587
Submission received: 30 September 2022
/
Revised: 31 October 2022
/
Accepted: 31 October 2022
/
Published: 4 November 2022
(This article belongs to the Special Issue Black Holes and Relativistic Jets)
Abstract
:We considered the fourth catalog of gamma-ray point sources produced by the Fermi Large Area Telescope (LAT) and selected only jetted active galactic nuclei (AGN) or sources with no specific classification, but with a low-frequency counterpart. Our final list is composed of 2980 gamma-ray point sources. We then searched for optical spectra in all the available literature and publicly available databases, to measure redshifts and to confirm or change the original LAT classification. Our final list of gamma-ray emitting jetted AGN is composed of BL Lac Objects (40%), flat-spectrum radio quasars (23%), misaligned AGN (2.8%), narrow-line Seyfert 1, Seyfert, and low-ionization nuclear emission-line region galaxies (1.9%). We also found a significant number of objects changing from one type to another, and vice versa (changing-look AGN, 1.1%). About 30% of gamma-ray sources still have an ambiguous classification or lack one altogether.
1. Introduction
The current paradigm of jetted active galactic nuclei (AGN) is mostly rooted in the seminal works by Rees, Schmidt, Blandford, Fanaroff, Riley, Orr, Browne, Barthel, Urry, Padovani, Ghisellini, just to cite a few [1,2,3,4,5,6,7,8,9]. Jetted AGN are basically divided into two main classes depending on the jet viewing angle (aligned with the Earth or not), which in turn are divided into two subclasses depending on the accretion rate. Flat-spectrum radio quasars (FSRQ) and BL Lac Objects have a small jet viewing angle, but the former have disks accreting at high rate, while the latter have weak and inefficient disks. They form the so-called blazar sequence, with FSRQs on one side, emitting high jet power, and BL Lac Objects on the opposite side, with low jet power. Misaligned AGN are commonly called radio galaxies, and are also divided according to the accretion rate into High-Excitation Radio Galaxies (HERG) and Low-Excitation Radio Galaxies (LERG). All these objects are powered by central supermassive black holes () hosted in giant elliptical galaxies (see [10] for a recent review).
However, the discovery of powerful relativistic jets from Narrow-Line Seyfert 1 galaxies (NLS1s) proved that the zoo of jetted AGN is more variegated than previously thought (see, for example, [11,12] for recent reviews). Although, NLS1s have been proven to be the low-luminosity tail of the FSRQs distribution [13], the relatively small mass of their central black hole and the high accretion rate implied that the blazar sequence no longer stands [14]. Therefore, it is important to keep the NLS1s classification separated from that of FSRQs, to avoid losing important physical information and implications, such as the second branch in the Jet-Disk plane (JD-plane), the branch of small-mass/high-accretion AGN [14].
Today, understanding the impact of NLS1s on the population of gamma-ray sources is hampered by the small number of known objects of this type ( [15]). In addition, recent studies on large samples are done by using computer-based procedures designed according to the old paradigm, which implies that this new class of objects is not recognized. Therefore, in order to have a large sample of gamma-ray emitting jetted AGN with updated and reliable optical classification and spectroscopic redshift, we performed the reclassification of the gamma-ray sources in the Fermi Large Area Telescope (LAT) (4FGL-DR2, [16], 4LAC, [17]) with extragalactic or unclassified counterparts (with the exclusion of starburst and normal galaxies), and outside the Galactic plane (). We collected 2980 gamma-ray point sources1. Then, for each source we searched for redshift measurements and optical spectra in the literature and data through the following public databases:
Preliminary results of this work (right ascension –, J2000) have been published in 2021 ([18], Paper I hereafter), and we refer to that paper for more details on the adopted procedures and explanations of the new classes of AGN.
2. Classification and Redshift
The full list of sources with their new classification is available in Appendix A. Table 1 summarizes the statistics of gamma-ray emitting jetted AGN after our reclassification, the fraction of sources with spectroscopic redshift, and the statistics from the original 4FGL-DR2 catalog. The sky distribution (Galactic coordinates, Aitoff projection) is shown in Figure 1. It is worth noting that there are some differences of classes between our classification and that of 4FGL, as explained in the notes of Table 1. We refer to Paper I for more details.
We also searched for photometric redshifts from a variety of catalogs and found at least one value for 2631 sources (88%, see Table A2). The complete (spectroscopic plus photometric) redshift distribution of sources is displayed in Figure 2. This information must be considered with care, because we noted some discrepancies between the coordinates of the counterparts given in the 4FGL and those available in radio databases. We generally considered valid the 4FGL coordinates, although we point out some cases of significant offsets (see also Section 3).
Although in Table A1 we include photometric redshifts only for the sources without a spectroscopic one (42% of the total sample), the availability of both measurements for a large sample of sources allowed us to give a rough estimation of the reliability of . As shown in Figure 3, there is some linear relationship between the two measurements for values smaller than one, but, for greater values, tends to be underestimated with respect to the spectroscopic measurements: while , the spectroscopic redshift reached values up to ∼4.3. Figure 4 displays the distribution of the difference , between photometric and spectroscopic redshifts: in most of cases, the photometric redshift is underestimated with respect to the spectroscopic one by .
It is also worth reporting the breakdown of our new classes, according to more common notations. For example, the MIS class contains 85 sources divided into: 8 Fanaroff-Riley type 0 (FR0), 35 FRI, 18 FRII, 7 compact steep-spectrum sources (CSS), and 1 steep-spectrum radio quasar (SSRQ). For the remaining 16 sources, we did not find publications with specific identification according to the above cited subclasses.
The AMB class contains a very heterogeneous set of sources, because the ambiguity can be due to different reasons:
- the difficulty to have a clear measure of the viewing angle, and so to distinguish between beamed and unbeamed jets (18 cases);
- different values of spectroscopic redshift, but no spectra published, making it impossible to choose the more reliable value (9);
- only a value of redshift without published spectra or any information about lines (3);
- Seyfert vs. NLS1, when no measurement of the full width half maximum (FWHM) of the H emission line is available (5);
- issues in the counterpart coordinates, see Section 3 (6);
- the possibility that the counterpart might be a Galactic source (1).
Further studies might solve these issues and change the number of objects in one class or another.
Most of CLAGN are beamed jetted AGN (30), transitioning from a featureless continuum to a line-dominated spectrum or vice versa, or displaying a change of the spectral energy distribution (e.g., J alias PMN J [19]). Three cases are misaligned AGN (J MS ; J PKS ; J 3C 216), and one curious case (J alias PKS ) refers to a change of the jet viewing angle, from a misaligned (MIS) to an aligned source (SEY) [20]. It is difficult to establish the real impact of CLAGN on the overall classification and population statistics, because most of the sources in the present sample do have only one optical spectrum. However, this is a very important point: the apparent classification is time-dependent and it would be desirable to move to more physics-based classifications.
3. Caveats
We have already pointed out some sources classified as AMB, because there were problems in the coordinates of the counterpart. For example, the 4FGL coordinates of the counterpart of J differ by from those of the gamma-ray centroid and located far outside the 95% error ellipse (). There is only one radio source inside the error ellipse of the gamma-ray source, so that we changed the 4FGL counterpart with this radio source and set the classification as AMB, because it needs more study to be confirmed or rejected.
It is worth citing another complex example: J is associated with NGC 7059, a nearby starforming spiral galaxy (). However, the 4FGL coordinates of the counterpart are not consistent with the center of the galaxy (difference ). These coordinates are consistent with a ROSAT source, 1RXS J (error radius , therefore not consistent with the galaxy center7). Swift follow-up of the gamma-ray source suggested a slightly different counterpart Swift J (distant from the ROSAT source), although consistent within the position errors with the ROSAT source [21,22]. However, at radio frequencies, there are two counterparts observed at 944 MHz with the Australian SKA Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU, [23]) Pilot Survey: one is consistent with the centroid of 1RXS J (∼2 mJy flux density and deconvolved size of ∼); the other is consistent with the centroid of Swift J (∼2.9 mJy flux density and is only barely resolved, ∼, J. Marvil, NRAO, priv. comm.). Therefore, more detailed studies are needed to assess the real counterpart of the gamma-ray source 4FGL J.
These examples show that sometimes we found inconsistencies between the name of the associated counterpart and its coordinates, but we decided to keep as reference the coordinates, and wrote potential issues in the notes. We also noted some minor differences (at arcsecond level) between the 4FGL coordinates and the values reported in radio catalogs, but again we kept 4FGL as reference, because this type of investigation is beyond our aims. However, we note that this discrepancy may affect the photometric redshifts reported in Table A2.
Another caveat refers to the classification. As previously stated, we made this reclassification almost completely according to the published information. This does not imply that it is carved into the stone. Particularly, large data sets cannot be analyzed directly by human being8 and require computer-aided procedures, which in turn—being prepared having in mind certain quantities and characteristics—can easily miss interlopers and outliers. Therefore, computer-aided analyses must be always verified, particularly if the spectrum displays strong noise or distortion of the line profiles.
The case of J (PKS , ) is exemplary: Shaw et al. [24] measured FWHM(H) km/s from a very noisy spectrum, with H barely visible and flooded in a strong background (the spectrum is available only in the online version of Shaw’s work9). The SDSS spectrum10 is a bit better, and clearly shows the H-[OIII] complex. Rakshit et al. [25] performed the measurement of the spectral properties of a large sample of AGN in the SDSS DR14. For PKS , they measured FWHM(H) km/s. Were these measurements correct, this AGN should be classified as NLS1, an unexpected and great result, because PKS was detected in 2015 at Very High Energies (VHE) by the MAGIC telescope [26]. Therefore, given the importance of the possible result, we reanalyzed the publicly available SDSS spectrum. The H profile is significantly distorted, with an apparent red wing, as like as the MgII. The line shape was decomposed into a narrow blue component and a broad red one. We measured FWHM(H) km/s for the former, and FWHM(H) km/s for the latter (see Figure 5), thus rejecting the NLS1 classification and to confirm the FSRQ one. These profiles can be fit with a relativistic accretion disk model oriented almost face-on, with ( is the gravitational radius), , inclination, emissivity exponent (continuum power law ), and local dispersion of H[27]. These parameters are consistent with their aligned classification, and with the current interpretation of the quasar main sequence [28,29]: for low FeII emission the line width is governed mainly by orientation (see Figure 3 of [30]). Similar cases of distorted emission-line profiles has been detected in many FSRQs and are likely due to low-ionization outflows [31] or gravitational redshift [32]. It is also worth noting that NLS1s do generally have Lorentzian profiles and the significant red wing apparent in the SDSS spectrum was another point against the NLS1 classification. To estimate the mass of the central black hole, it is better to use the [OIII], given the significant distortion of the H line profile. We measured a FWHM([OIII]) km/s and, by applying the relationship [33] (see also Equation (6) in [34]), we can estimate , which is typical for FSRQs.
We already started a parallel follow-up program to reanalyze the publicly available optical spectra for the NLS1 and SEY classes, and to ask for new high-quality observations. The new data, when available, will be reported elsewhere. Here we just want to remind that the present results have to be taken cum grano salis.
Last, but not least, works like the present one never end. New observations can improve or reject the current classification and the gamma-ray sky is still an effervescent research field, so that new papers are published at a non-negligible rate. The present work includes information published until 30 August 2022.
4. Comparison with CGRO/EGRET
The present reclassification resulted in 24 NLS1s and 32 Seyfert/LINERs candidates or confirmed ones. Therefore, it is rather obvious to wonder if Seyfert-type AGN could have been detected by the EGRET instrument onboard the Compton Gamma-Ray Observatory. Although it is expected that the jet power of highly-accreting small-mass black holes hosted by NLS1s scales with [35], it is also known that strong gamma-ray outbursts have been observed from NLS1 by Fermi/LAT, with fluxes exceeding ∼ ph cm s at energies greater than 100 MeV (e.g., [36,37,38,39]). These values are within the capabilities of CGRO/EGRET. Therefore, we cross-matched our reclassified list of gamma-ray sources with the Third EGRET Catalog [40] by using an error circle of one degree. We found 100 matches, subdivided into 54 FSRQ, 30 BLLAC, 2 NLS1, 2 MIS, 1 AMB, 3 CLAGN, and 8 UNCL.
The two NLS1 are:
- 4FGL J = 3EG J: in this case, the EGRET source was originally associated with the FSRQ TXS (), while the LAT source, with an improved error circle, has a different counterpart, TXS (). The SDSS spectrum11 of the latter clearly displays a H with a Lorentzian profile and the FeII bumps. The analysis by Wu & Shen [41] resulted in FWHM(H) km/s and an estimated mass of the central black hole of ∼.
- 4FGL J = 3EG J: the gamma-ray source is associated in both cases with PKS (), which was classified as AGN [40], and later as FSRQ [42]. Shaw [24] measured FWHM(H) km/s, formally NLS1, but the error is so large to cast significant doubts. A multiwavelength study of this jetted AGN favoring the NLS1 classification has been recently presented by Jessica Luna at the workshop Panchromatic View of the Life-Cycle of AGN (14–16 September 2022, ESA/ESAC, Spain)12. However, an optical spectrum with better S/N is needed to confirm this classification.
It is also worth noting another case: 4FGL J = 3EG J, associated with the FSRQ TXS () by EGRET and to a different counterpart by LAT, TXS (). For the latter, we found three measurements of the FWHM(H): km/s [24], km/s [25], and km/s [41]. Therefore, Shaw’s measurement suggested it might be a NLS1, but a quick look at the SDSS spectrum13 shows evident red wings in the profiles of MgII and H, although the latter is strongly affected by noise. It seems to be a case similar to PKS , outlined in the previous section, which implies a FSRQ classification.
To summarize, in the first case the finding of a NLS1 was not possible because of a poor EGRET contours probability, which in turn led to a wrong counterpart, while in the second one, the counterpart is the same as for LAT, but a reliable optical spectrum is still missing to confirm the classification. These few possible detections can be explained by the smaller field of view (FOV) of EGRET14 (∼0.5 sr vs. >2 sr of LAT), which means that almost pointed observations were required to catch a flare of a NLS1. On the opposite, Fermi/LAT, with its large FOV and excellent sensitivity, can scan the entire sky every three hours, implying a significant increase of the probability to detect an outburst from Seyfert-type jetted AGN.
5. The Twilight Zone
The manual screening of such a large sample of cosmic sources gave us the opportunity to observe many unusual features of these objects. Among the most interesting cases, there are:
- 4FGL J = PKS B: the jetted AGN is behind a Seyfert 2 galaxy at [43];
- 4FGL J = B3 : the SDSS image15 shows the object forming something like a circle with other apparently close objects, perhaps an Einstein ring?;
- 4FGL J = SBS : this jetted AGN is a Seyfert hosted in a spiral galaxy, where a SNII exploded in 2009 (2009fe, see Figure 15 in [44]);
- 4FGL J = S3 : it is a triple interacting system [45];
- 4FGL J = 4C : originally classified as BL Lac Object, because of small equivalent width emission lines, once the host galaxy continuum is removed, it clearly displays a Seyfert-1 spectrum (see Figure 4 in [46]);
- 4FGL J = PKS : tidal interaction with a close companion, precessing jet [47];
6. Final Remarks
We presented a list of 2980 gamma-ray sources from the Fourth Fermi LAT point-source catalog, with revised classification and spectroscopic or photometric redshift. The main result is that the gamma-ray emitting jetted AGN zoo is more variegated than previously thought, with emerging populations of Seyfert-type AGN. It is also worth noting that an AGN can change classification with time on human time scales, because of intrinsic changes in the emission mechanisms.
We would like to stress that users should read the literature thoroughly before using their data and conclusions. A simple cross-match of catalogs at different frequencies is not sufficient. A lot of high-level information (which can be found only in published papers, because it required a human analysis) can be missed, with significant impact on the knowledge about the nature of these cosmic sources. In addition, as we already noted in the Paper I, online databases may not be updated with the most recent findings or occasionally contain plain errors.
Author Contributions
Conceptualization, L.F.; Writing—Original Draft, L.F.; and Writing—Review and Editing, L.F., M.L.L., H.A., S.C., P.M., S.A., M.B., E.D.B., E.J., M.J.M.M., P.R., M.T., S.V. and A.V. All authors have read and agreed to the published version of the manuscript.
Funding
H.A. benefited from support via CIIC 138/2022 of Universidad de Guanajuato, Mexico.
Data Availability Statement
The list of sources is available in Appendix A. All the publicly available data and published references can be accessed through the hyperlinks. Photometric redshifts are available in Table A2.
Acknowledgments
We thank Marco Simonte for help with the extraction of photometric redshift values from NOIRlab. Funding for the Sloan Digital Sky Survey (SDSS) was provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the U.S. Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society. The SDSS Web site is http://www.sdss.org/ (accessed on 30 August 2022). The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The Participating Institutions are the University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, Los Alamos National Laboratory, the Max–Planck–Institute for Astronomy (MPIA), the Max–Planck–Institute for Astrophysics (MPA), New Mexico State University, University of Pittsburgh, Princeton University, the United States Naval Observatory, and the University of Washington. Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. This research made use of the SIMBAD database, operated at CDS, Strasbourg, France (2000, A&AS, 143, 9, “The SIMBAD astronomical database”, Wenger et al.). This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in 2000, A&AS 143, 23. This research made use of the NASA/IPAC Extragalactic Database (NED), which is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology. This research made use of NASA’s Astrophysics Data System Bibliographic Services.
Conflicts of Interest
The authors declare no conflict of interest.
Appendix A. List of Gamma-Ray Emitting Jetted Active Galactic Nuclei
Column explanation for Table A1:
- 4FGL-DR2 name (JHHHH.H ± DDDD);
- 4FGL-DR2 counterpart;
- Right Ascension (J2000) of the counterpart [deg];
- Declination (J2000) of the counterpart [deg];
- Redshift (max 3 significant digits);
- Reference where the first measurement of z is reported;
- 4FGL-DR2 original classification (see the 4FGL catalog paper for explanation);
- Revised classification, based on optical spectra:
- FSRQ: Flat-Spectrum Radio Quasar;
- BLLAC: BL Lac Object;
- NLS1: Narrow-Line Seyfert 1 Galaxy;
- SEY: Seyfert galaxy (Type 1, 2, intermediate, LINER);
- MIS: Misaligned Jetted AGN;
- CLAGN: Changing-look AGN;
- AMB: ambiguous;
- UNCL: unclassified;
see Paper I for details and explanation of the proposed classification; - Flag for the redshift:
- 0: spectroscopic redshift;
- 1: non-spectroscopic redshift (photometric, imaging of the host galaxy, cross-correlation with zero-velocity template, from nearby galaxies in a cluster);
- 2: featureless/inconclusive spectrum;
- 3: no optical data found;
- Notes
- Radio spectral indexes () are mostly from Specfind (Vollmer+ 2009) or calculated by using SED data from NED (, flat or inverted spectrum; , steep spectrum);
- If zFlag=1 or 2, then the reference is to the latest optical spectrum, unless specified otherwise.
Please note that the hyperlinks open directly the web pages with the full-text articles from NASA/ADS or publicly available optical spectra. All hyperlinks have been accessed for a check on 30 August 2022.
Table A1.
See the text for explanation.
| 4FGL Name | 4FGL Counterpart | RA | DEC | z | Reference for z | Cl | R-Cl | zFlag | Notes |
|---|---|---|---|---|---|---|---|---|---|
| J | B3 | 0.545 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.382 | Table A2 | bll | BLLAC | 1 | Shaw+(2013) | ||
| J | TXS | 0.439 | Muñoz+(2003) | fsrq | NLS1 | 0 | SIMBAD and NED reported an old by Falco+(1998) based on the lines [CIII], Ne V, He I. Muñoz is based on Ne IV, Mg II, He I, [OIII]. SDSS confirms Muñoz+(2003) value. It also shows the H-[OIII] complex, with evident FeII bumps on both sides, and Wu+Shen (2022) measured FWHM(H) km/s. The profile of H is enlarged toward the basis, suggesting it might be an intermediate Seyfert. | ||
| J | 2MASS J | 0.290 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.219 | Table A2 | bcu | BLLAC | 1 | Desai+(2019) | ||
| J | WISEA J | 0.545 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISE J | 0.717 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 6 | 0.309 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.711 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.636 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.519 | Table A2 | bll | BLLAC | 1 | Healey+ (2008) | ||
| J | SDSS J | 1.36 | Table A2 | bcu | BLLAC | 1 | Paiano+ (2019) | ||
| J | MG4 J | 1.81 | Sowards-Emmerd+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.880 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 0.229 | Stickel & Kühr (1994) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.347 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.787 | Paiano+ (2019) | bcu | BLLAC | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | MG4 J | 2.32 | Table A2 | bll | BLLAC | 1 | Both NED and SIMBAD give from Kock+ (1996), but this value is based on a partial and featureless spectrum. Kock suggested that value on the basis of two possible absorption features from the host galaxy (G-band, Na). Never confirmed. Paiano+ (2017) still found a featureless spectrum. | ||
| J | PMN J | 1.33 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.07 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 16 | 0.147 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.682 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.589 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | IC 1531 | 0.0256 | da Costa+ (1991) | rdg | MIS | 0 | FRI, Bassi+ (2018) | ||
| J | RX J | 0.471 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.200 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | TXS | 0.598 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.19 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.17 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 1.49 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.834 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.944 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.434 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 1RXS J | 0.226 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 0.255 | Thompson+ (1992) | agn | MIS | 0 | Thompson+ (1992) measured the redshift on the basis of [OIII] line and suggested a classification as NELRG. Véron-Cetty & Véron (2010) classify it as Seyfert 1.9, thus confirming an obscured object at large viewing angle. Kayanoki+Fukazawa (2022) classified it as FRII. | ||
| J | PKS | 1.08 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | RBS 30 | 0.0948 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | MG3 J | 0.477 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | RBS 32 | 0.176 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | MS | 0.163 | SDSS | bll | CLAGN | 0 | The SDSS spectrum displays evident lines (H+NII, [OIII]), but Rector+ (1999) published a very different spectrum (featureless, see Figure 5), although it measured the same redshift via absorption features of the host galaxy. Rector also reported a FRI classification (MIS) on the basis of VLA radio maps. | ||
| J | GALEXASC J | 0.791 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 3C 6 | 0.414 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.491 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007) | ||
| J | GB6 J | 0.485 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | S3 | 1.58 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 1.72 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.357 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.227 | Healey+ (2008) | FSRQ | FSRQ | 0 | - | ||
| J | GB6 J | 0.303 | SDSS | bll | BLLAC | 0 | - | ||
| J | RBS 42 | 0.1 | Fischer+ (1998) | bll | BLLAC | 1 | - | ||
| J | PMN J | 0.522 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | PKS | 0.775 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | S5 | 1.78 | Lawrence+ (1996) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.652 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 0.390 | Table A2 | bll | BLLAC | 1 | Titov+ (2017) | ||
| J | NVSS J | 0.648 | SDSS | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.25 | Arsioli+ (2015) | bll | BLLAC | 1 | - | ||
| J | RX J | 0.306 | Brinkmann+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | 1RXS J | 0.856 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) indicated on the basis of absorption features identified as an intervening system, while Ackermann+ (2016) suggested that those features are of the host galaxy and, therefore, set . | ||
| J | PKS | 2.86 | Truebenbach & Darling (2017) | bll | BLLAC | 0 | - | ||
| J | B3 | 1.06 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.354 | Mahony+ (2011) | bcu | MIS | 0 | Callingham+ (2017) reported the peak of radio emission at 177 MHz. Steep radio spectrum (). | ||
| J | 87GB | 0.732 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B3 | 1.44 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.546 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.834 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.554 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Thomas+ (1998) | ||
| J | GB6 J | 1.00 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.55 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.0828 | SDSS | bll | SEY | 0 | FRI radio morphology (Capetti+ 2019), but flat radio spectrum of the core (Healey+ 2007). | ||
| J | GB6 J | 0.581 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | NVSS J | 0.257 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.237 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.495 | Hook+ (2003) | fsrq | FSRQ | 0 | SIMBAD reports from Hewitt & Burbidge (1989), which in turn is from Savage (1984): she reported two emission lines at 4120 and 5080 Å identified as CIV and CIII]. No spectrum is published. Hook published the spectrum, where the two lines are identified as MgII and [NeV], respectively. Other lines are reported ([NeIII], H, H), confirming . | ||
| J | PKS B | 1.80 | SDSS | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.827 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | SUMSS J | 1.19 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.324 | Landt & Bignall (2008) | bll | BLLAC | 0 | - | ||
| J | RBS 75 | 0.0727 | Schwope (2000) | bll | BLLAC | 0 | - | ||
| J | KUV | 0.936 | Table A2 | bll | BLLAC | 1 | Both SIMBAD and NED indicated from Giommi+ (2005), which in turn refer to Bauer+ (2000) and Piranomonte+ (2007). The former did not indicate any redshift and classify it as BL Lac Object, while the latter reported an uncertain from an unpublished featureless spectrum with a weak EW. Shaw+ (2013) and Pita+ (2014) still found featureless spectra. | ||
| J | MG3 J | 0.743 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.14 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.272 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.721 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | PMN J | 0.965 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 1.59 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 4C | 0.366 | Vermeulen & Taylor (1995) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.0890 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | WISE J | 0.148 | Falco+ (1998) | bll | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.532 | Table A2 | bll | BLLAC | 1 | Both NED and SIMBAD give based on Croom+ (2009), which in turn used a SDSS spectrum and marked it as not reliable. Additionally, a more recent SDSS spectrum is inconclusive. | ||
| J | PKS | 0.498 | Jones+ (2009) | fsrq | FSRQ | 0 | 6dF. Jauncey+ (1984) reported on the basis of three weak emission lines (spectrum unpublished). The two spectra have a partial overlap (6dF, Å; Jauncey, Å) and only one line in common at 4195 Å, which is identified as MgII by Jones, and CIII] by Jauncey. Since the FWHM is quite large (Jauncey reported km/s), the MgII identification seems to be the more likely. | ||
| J | 3C 17 | 0.220 | Schmidt (1965) | rdg | MIS | 0 | SDSS. FRII, Balmaverde+ (2019). | ||
| J | TXS | 2.10 | Sowards-Emmerd+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.541 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.0644 | Vettolani+ (1989) | bcu | BLLAC | 0 | Loveday (1996) classified the host galaxy as lenticular (S0). | ||
| J | B3 | 0.295 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | PMN J | 0.213 | Landt & Bignall (2008) | bll | BLLAC | 0 | The authors referred to an unpublished spectrum and flagged it as uncertain, but the value was later confirmed by Marchesini+ (2019). | ||
| J | TXS | 0.632 | SDSS | bcu | FSRQ | 0 | - | ||
| J | B3 | 0.380 | Fittingoff+ (2009) | fsrq | FSRQ | 0 | - | ||
| J | RBS 97 | 0.150 | Schwope+ (2000) | bcu | BLLAC | 0 | - | ||
| J | RX J | 0.524 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007) | ||
| J | PKS | 1.43 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 1.42 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.604 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.264 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.966 | Shaw+ (2012) | fsrq | FSRQ | 0 | The automatic pipeline of the SDSS spectrum suggest , on the basis of a feature identified as Ly. The same feature was identified by Shaw+ (2012) as Mg II. | ||
| J | PKS | 1.03 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.03 | Klindt+ (2017) | bcu | FSRQ | 0 | - | ||
| J | GB6 J | 0.425 | Paiano+ (2020) | bll | BLLAC | 0 | SDSS | ||
| J | GB6 J | 0.255 | Paiano+ (2020) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 1.16 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | B3 | 0.252 | Djorgovski+ (1995) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.364 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 0.264 | SDSS | bll | MIS | 0 | In a cluster. Steep radio spectrum with detection at 74 MHz (VLSS), but Liu & Zhang (2002) reported a one-side jet: head-tail radio galaxy? | ||
| J | GALEXASC J | 0.302 | Paiano+ (2017) | bcu | BLLAC | 0 | - | ||
| J | PMN J | 0.168 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | SUMSS J | 0.286 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.121 | Schectman+ (1996) | bcu | SEY | 0 | Schwope+ (2000) classified it as Seyfert. | ||
| J | PKS | 1.47 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.80 | Peterson+ (1976) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.920 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.635 | Shaw+ (2013) | BLL | BLLAC | 0 | - | ||
| J | PKS | 1.98 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.168 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | PKS | 1.75 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | MIS | 3 | MIS (composite) from Australia Telescope Low-Brightness Survey (ATLBS) by Subrahmanyan+ (2010). Steep radio spectrum. | ||
| J | WN B | 0.894 | Table A2 | bcu | UNCL | 1 | - | ||
| J | FRBA J | 0.313 | Table A2 | bll | BLLAC | 1 | SIMBAD gives from Neronov+ (2015), who in turn did not give any reference. Featureless spectra are reported by Masetti+ (2013) and Shaw+ (2013). | ||
| J | TXS | 1.07 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.34 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.103 | SDSS | bll | MIS | 0 | FRI, head-tail, Miraghaei & Best (2017). | ||
| J | PMN J | 0.442 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.263 | Peña-Herazo+ (2021) | bcu | AMB | 0 | Classified as double radio source by Zanichelli+ (2001), but without further specific notes. Flat radio spectrum: BLLAC? Vettolani+ (1998) reported , but no spectrum published. | ||
| J | PKS | 0.385 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | CRATES J | 0.317 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.206 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | - | ||
| J | 87GB | 0.558 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.707 | Table A2 | bcu | BLLAC | 1 | Healey+ (2008) | ||
| J | NGC 315 | 0.0167 | Colla+ (1975) | rdg | MIS | 0 | Classified as FRI by Venturi+ (1993). Barth+ (1999) classified it as LINER 1.9 in an elliptical galaxy. | ||
| J | PKS | 1.25 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.320 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | RX J | 0.286 | Table A2 | bll | UNCL | 1 | - | ||
| J | MG3 J | 1.37 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.719 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.144 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS | ||
| J | PKS B | 0.874 | Tinney (1999) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.284 | Table A2 | bll | BLLAC | 1 | Mahony+ (2010) | ||
| J | GB6 J | 0.983 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.545 | Table A2 | bll | BLLAC | 1 | SDSS. Ching+ (2017) suggested on the basis of SDSS-DR7 spectrum. | ||
| J | MRSS | 0.261 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PKS | 1.02 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.549 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.421 | Paiano+ (2017) | bcu | BLLAC | 0 | SDSS | ||
| J | GB6 J | 0.874 | Shaw+ (2012) | fsrq | NLS1 | 0 | Shaw+ (2012) reported FWHM(H) km/s. | ||
| J | PKS | 0.386 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.37 | Rajagopal+ (2021) | bcu | BLLAC | 0 | - | ||
| J | GB6 J | 0.832 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.246 | SDSS | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.490 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.747 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.440 | Shaw+ (2013) | bll | BLLAC | 0 | Marlow+ (2000) reported on the basis of two possible lines (H, [OII]), but they themselves flagged it as uncertain. The value measured by Shaw+ (2013) is based on features of the host galaxy. | ||
| J | PMN J | 0.662 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.307 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | PMN J | 0.869 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.37 | Strittmatter+ (1974) | fsrq | FSRQ | 0 | SDSS | ||
| J | 4C | 2.11 | Burbidge (1968) | fsrq | FSRQ | 0 | SDSS | ||
| J | MG1 J | 0.444 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS. NED reports from Bauer+ (2000). However, it is not possible to find that spectrum in order to understand how they estimated z and no specific notes are available in their paper. | ||
| J | GB6 J | 0.493 | SDSS | bcu | BLLAC | 0 | - | ||
| J | RBS 158 | 0.313 | Fischer+ (1998) | bll | BLLAC | 0 | - | ||
| J | 6C B | 0.0960 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.234 | Fischer+ (1998) | bll | BLLAC | 1 | - | ||
| J | 1RXS J | 0.347 | Nass+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 1.47 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.19 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | S2 | 0.265 | Healey+ (2008) | BLL | BLLAC | 0 | This result was challenged by Paiano+ (2008), who reported a featureless spectrum. However, Paiano reported , brighter than reported by Healey. It is likely that jet activity has hidden the weak features observed by the latter. The galaxy is far from S2 reported by Paiano, with redshift similar to Healey’s, is likely to be in the same cluster, but it has . Even it falls in the slit, it cannot contaminate the spectrum of S2 (3 mag difference). The conclusions of Paiano are challenged by their own Figure 5: they wrote that the Ca H&K break can disappear for , but in that case R would have been , while they reported . Therefore, it is likely that they did not observe the calcium break simply because of an increased jet activity, while Healey observed the weak features because the object was in low optical state. | ||
| J | TXS | 0.772 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.480 | Chang+ (2019) | bll | BLLAC | 1 | - | ||
| J | 4C | 0.603 | Wills & Wills (1976) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.3 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 1.22 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 0.389 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | UGC 773 | 0.0470 | Wills & Wills (1976) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.583 | Stadnik & Romani (2014) | bll | BLLAC | 1 | - | ||
| J | 1RXS J | 0.482 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 1.15 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 1.37 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.483 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | RX J | 0.376 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.671 | Wright+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.432 | Table A2 | bll | BLLAC | 1 | Croom+ (2004) | ||
| J | SUMSS J | 0.169 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | 1RXS J | 0.296 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) | ||
| J | PKS | 1.41 | Croom+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.279 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.49 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | AT20G J | 1.64 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.16 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.187 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | PKS | 0.639 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASX J | 0.109 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | CRATES J | 1.19 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.408 | Table A2 | bll | BLLAC | 1 | Falomo (1989) | ||
| J | 2MASS J | 0.839 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.390 | Peña-Herazo+ (2017) | bcu | BLLAC | 0 | - | ||
| J | 1RXS J | 0.567 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1ES | 0.272 | Perlman+ (1996) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.404 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | PMN J | 2.12 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.24 | Table A2 | bll | BLLAC | 1 | Titov+ (2011) | ||
| J | MG3 J | 1.26 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.28 | MacAlpine & Feldman (1982) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.717 | Baker+ (1999) | fsrq | FSRQ | 0 | - | ||
| J | WISEA J | 0.988 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.524 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007) | ||
| J | NVSS J | 0.284 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | PMN J | 0.419 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.866 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.0670 | Marcha et al. (1996) | bll | AMB | 0 | Rather strange object, a hybrid between BL Lac object and FRI, according to Marcha+ (1996) and Jackson+Marcha (1999). The optical spectrum shows H+[NII] and [OIII] lines, but not H, suggesting the presence of partial covering, and hence a large viewing angle. LAT spectrum is rather soft () favoring the MIS classification, rather than BLLAC. Lister classified it as radio galaxy in their MOJAVE project. Antón+Browne (2005) reported a brightness temperature at 5 GHz of K. | ||
| J | GB6 J | 0.228 | Marlow+ (2000) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.690 | Table A2 | bcu | AMB | 1 | SDSS inconclusive. Radio morphology from Douglas+ (1996) is symmetric double with lobes, but the TGSS indicates a point-source. The radio spectrum from SIMBAD/Specfind is steep, but the TGSS-NVSS slope is inverted. | ||
| J | 4C | 1.63 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | MG1 J | 0.768 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 0.149 | Bauer+ (2000) | bcu | SEY | 0 | Bauer+ also classified it as Sy 1.5. | ||
| J | PKS | 1.02 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 1.19 | Table A2 | bcu | BLLAC | 1 | Henstock+ (1997) | ||
| J | SUMSS J | 0.151 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | PKS | 0.925 | Marchesini+ (2019) | bcu | FSRQ | 0 | Johnston+ (1995) reported of unknown origin. | ||
| J | 1RXS J | 0.682 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 2.14 | Iovino+ (1996) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.571 | Marchesi+ (2018) | fsrq | CLAGN | 0 | This source is rather intriguing and would deserve further studies. Shaw+ (2013) and Paiano+ (2020) reported featureless spectra and classified it as BL Lac object, with lower limits for z ( for Paiano; she also suggested that the MgII line reported by Marchesi is an artifact). However, Marchesi+ (2018) found a prominent emission line at 4400 Å, which is identified as Mg II. Therefore, they measured and classified the source as FSRQ. The SDSS spectrum is featureless. The instruments used by Shaw and Paiano started from 4150 Å, while Marchesi and SDSS started from 3500 Å. The observations dates are: 14 October 2010, Shaw; 2 February 2015, SDSS; 10 October 2017, Marchesi; 3 December 2017, Paiano. The variability expected from a jetted AGN can explain differences in spectra from observations separated by years. Even the two months of separation from Marchesi and Paiano observations could be still well explained in terms of source variability. In addition, it is worth noting that the expected feature at 4400 Å is close to the lower wavelength boundary of the instrument used by Paiano, although the EW measured by Marchesi (EW = 64 Å) would make it measurable even with low instrument performance. Last, but not least, the other spectra collected on the same night by Marchesi did not record any signal on the same wavelength. Anyway, this source deserves a monitoring campaign. It might be a case similar to PMN J2345−1555. | ||
| J | 1RXS J | 0.372 | SDSS | bcu | BLLAC | 0 | - | ||
| J | B3 | - | - | bll | BLLAC | 2 | Featureless, the latest observation was done by Paiano+ (2017). SIMBAD reported from Neronov+ (2015), but it seems to be the lower limit measured by Shaw+ (2013). | ||
| J | OC 457 | 0.859 | Lawrence+ (1986) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.837 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.715 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.0901 | Jones+ (2009) | bcu | BLLAC | 0 | - | ||
| J | WISE J | 0.347 | SDSS | bll | BLLAC | 0 | - | ||
| J | WN B | 0.777 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.300 | Table A2 | bll | BLLAC | 1 | Sbarufatti+ (2009) | ||
| J | PKS | 0.733 | Stocke+Rector (1997) | bll | BLLAC | 0 | Stocke+Rector (1997) reported an absorption line MgII at , and two weak emission lines (MgII, [OII]) at . This value is confirmed by Shaw+ (2013), but not by Paiano+ (2020), likely due to jet activity. SDSS inconclusive. | ||
| J | PKS | 0.377 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013) | ||
| J | PMN J | 0.865 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.375 | Croom+ (2004) | bcu | FSRQ | 0 | See also Londish+ (2007) for the classification as Type 1 AGN. | ||
| J | SUMSS J | 0.027 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | TXS | 0.675 | Table A2 | bll | BLLAC | 1 | Shaw+ (2009) | ||
| J | PKS | 1.15 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.922 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | SUMSS J | 0.229 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | B3 | 0.592 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.0981 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.940 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.722 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.188 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.609 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | WN B | 0.150 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.198 | Table A2 | bcu | UNCL | 1 | The 3FGL (Ackermann+ 2015) reported , but there is no information on the origin of this measurement. No references on optical spectra are available neither on SIMBAD nor on NED. | ||
| J | PKS | 1.32 | Wampler+ (1984) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 | 0.55 | Table A2 | bcu | UNCL | 1 | The 3FGL (Ackermann+ 2015) gives , but there are no information about the origin of this measurement. No other published papers with any spectroscopic redshift measurement. | ||
| J | PMN J | 0.080 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 2.35 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.58 | Eracleous+Halpern (1994) | fsrq | FSRQ | 0 | Savage+Bolton (1979) reported , but without information. | ||
| J | GB6 J | 0.681 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.0823 | Jones+ (2009) | bcu | BLLAC | 0 | - | ||
| J | GB6 J | 0.856 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | 0.437 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.08 | Nass+ (1996) | bcu | BLLAC | 1 | - | ||
| J | MG4 J | 0.446 | Peña-Herazo+ (2021) | bcu | FSRQ | 0 | LAMOST | ||
| J | PMN J | 0.261 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.117 | Table A2 | bll | UNCL | 1 | - | ||
| J | MG4 J | 0.972 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.304 | Goldoni+ (2021) | bll | BLLAC | 0 | - | ||
| J | PMN J | 2.29 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.233 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | GB6 J | 0.454 | Paiano+ (2019) | fsrq | BLLAC | 0 | - | ||
| J | PMN J | 0.812 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.195 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.453 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 1RXS J | 0.0539 | Jones+ (2009) | bcu | BLLAC | 0 | - | ||
| J | PMN J | 1.28 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | MS | 0.298 | Stocke+ (1991) | bll | BLLAC | 0 | SDSS | ||
| J | GALEXASC J | 0.610 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.629 | Shaw+ (2012) | fsrq | BLLAC | 0 | - | ||
| J | WISE J | 1.35 | Becker+ (2001) | fsrq | FSRQ | 0 | SDSS | ||
| J | B3 | 0.94 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | RX J | 0.142 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S5 | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | NVSS J | 0.761 | SDSS | bll | FSRQ | 0 | - | ||
| J | 1RXS J | 0.617 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.740 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.210 | de Menezes+ (2020) | bcu | BLLAC | 0 | - | ||
| J | 4C | 0.405 | Perlman+ (1998) | bcu | FSRQ | 0 | Classified as CSS quasar, An+ (2016), but SPECFIND gives a rather flat spectrum . The value of redshift was challenged by Jones+ (2018), which referred to Stickel+ (1996). Stickel reported on the basis of two lines identified as [OII] and [NeII]. The same lines were identified by Perlman as H and [OIII], together with other lines in the spectrum (H). Additionally, Olguín Iglesias+ (2016) supported the Perlman’s redshift on the basis of the study of the host galaxy. | ||
| J | PKS | 1.74 | Kinman+ (1967) | fsrq | FSRQ | 0 | The first value is reported by Kinman+ (1967), who in turn referred to a spectrum taken by Arp with 200-inches at Mt Palomar. However, neither data nor value are reported. Anyway, the value of redshift has been confirmed later by many authors (e.g., 6dF). | ||
| J | B2 | 1.47 | Burbidge (1970) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.66 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.188 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.254 | Machalski+Condon (1999) | bcu | BLLAC | 0 | Classified as BLLAC by Peña-Herazo+ (2021), who also confirmed the redshift. | ||
| J | PMN J | 0.582 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.595 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | PKS | 0.684 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MS | 0.351 | Watson+ (2004) | bll | BLLAC | 0 | There was a debate about the redshift, because the early identification with a spiral host galaxy was wrong (first value of z in Stocke+ 1991; BL Lac off center of the spiral host in Stocke+ (1995), spiral in foreground, microlensing suggested). Falomo+ (1997) found a nebulosity coincident with the BL Lac object, which was identified as an elliptical galaxy and strengthened Stocke’s value. Watson’s value was derived from the detection of an MgII absorption doublet. | ||
| J | 1RXS J | 0.268 | Table A2 | bll | BLLAC | 1 | Bauer+ (2000) | ||
| J | PMN J | 0.211 | Goldoni+ (2021) | bll | BLLAC | 0 | - | ||
| J | S5 | 0.895 | Vermeulen+ (1996) | bll | FSRQ | 0 | - | ||
| J | GB6 J | 0.276 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.00 | Wilkes+ (1983) | FSRQ | FSRQ | 0 | - | ||
| J | NVSS J | 1.26 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 0.200 | Meisner+Romani (2010) | BLL | BLLAC | 1 | - | ||
| J | RX J | 0.169 | SDSS | bcu | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | RBS 292 | 0.393 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.565 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG3 J | 0.459 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | 2MASS J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.172 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PMN J | 1.2 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.174 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.450 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.735 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WN B | 0.107 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.408 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | RBS 298 | 0.288 | Fischer+ (1998) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.737 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.14 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | RBS 300 | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | PKS | 0.607 | Shaw+ (2012) | fsrq | AMB | 0 | SDSS spectrum is a bit noisy, with weak and narrow lines suggesting partial covering. Radio spectrum is flat; Gamma-ray spectrum is soft. Could be SEY or NLS1. | ||
| J | ZS | 0.0850 | Shaw+ (2013) | bll | BLLAC | 0 | Gorshkov+Konnikova (1983) earlier suggested a quasar classification and , but they themselves recognized it could be a spurious identification given the weakness of the lines. | ||
| J | S5 | 2.37 | Lawrence+ (1986) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.72 | Foltz+ (1987) | fsrq | CLAGN | 0 | Early detections suggested a BL Lac identification, with featureless spectrum and many absorption lines due to intervening systems. The first estimate of the redshift was by Blades+ (1985), who identified the Ly forest. Then, Foltz+ (1987) detected two emission lines (SiIV, CIV), consistent with Blades’ estimates. The equivalent width of CIV (18Å) points to a FSRQ classification, but also to a changing-look AGN. It is worth noting that the BL Lac-type spectrum was taken when the source was faint, while the FSRQ-type spectrum was observed when the source was bright. This seems to be due to a change in the accretion rate rather than to the jet activity. | ||
| J | MG3 J | 1.07 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.685 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.489 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | 1RXS J | 0.128 | Wolter+ (1998) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.934 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | CRATES J | 1.62 | Hook+ (1996) | fsrq | FSRQ | 0 | There is a typo in the counterpart name in the 4FGL: it is written CRATES J022048+324116, but it should be CRATES J022048 + 324106. | ||
| J | RX J | 0.525 | Smith+ (2007) | bll | BLLAC | 0 | - | ||
| J | B2 | 0.944 | Cohen+ (2003) | FSRQ | FSRQ | 0 | Gravitationally lensed object by an object at . NED erroneously reports this latter value for z. | ||
| J | TXS | 0.850 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.543 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.923 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.698 | Wilkes+ (1986) | fsrq | FSRQ | 0 | - | ||
| J | 3C 66A | 0.340 | Torres-Zafra+ (2018) | BLL | BLLAC | 1 | Long-standing debate on the value of z because all the taken spectra are almost featureless. Bu+ (2019) reported a hint of Ly (2.2 with HST/COS) consistent with the expected redshift. | ||
| J | PKS | 1.49 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.518 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | PKS | 1.01 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 1.22 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.00 | SDSS | bcu | FSRQ | 0 | - | ||
| J | GALEXASC J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bll | UNCL | 3 | - | ||
| J | PKS | 0.511 | White+ (1988) | fsrq | NLS1 | 0 | FWHM(H) = 27Å km/s, and strong [OIII], flat radio spectrum, soft gamma-ray spectrum. | ||
| J | NVSS J | 0.887 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 2.69 | Schwope+ (2000) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.917 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.437 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.466 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.68 | Titov+ (2017) | bcu | FSRQ | 0 | Warning: SIMBAD coordinates are wrong (difference ). | ||
| J | NVSS J | 0.788 | Table A2 | fsrq | UNCL | 1 | - | ||
| J | RBS 318 | 0.380 | Table A2 | bll | BLLAC | 1 | Jones+ (2009) | ||
| J | PMN J | 0.013 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.373 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 1.57 | Vigotti+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.457 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.514 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.303 | Croom+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | WN B | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.401 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.46 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.734 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.11 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 1.02 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.765 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.0320 | Fairall (1980) | bll | BLLAC | 0 | Host galaxy SB type with inner ring (Buta 1995). | ||
| J | 4C | 2.06 | Schmidt (1968) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.209 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | 1ES | 0.140 | Schachter+ (1993) | bll | BLLAC | 0 | - | ||
| J | B2 | 0.531 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.127 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.225 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 1.13 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.687 | Table A2 | bll | BLLAC | 1 | Paiano+ (2019) | ||
| J | PHL 1389 | 1.55 | Table A2 | bll | UNCL | 1 | Croom+ (2004) found (quality flag 11, high-quality spectrum, no more available) and classified it as a star. Additionally, Kilkenny+ (2016) classified it as B/sdB star. Could the -ray emission be due to a XRB with a neutron star? Arsioli+ (2015) suggest it could be a BL Lac object with . | ||
| J | PKS | 0.465 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | OD 58 | 0.335 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 334 | 0.411 | Pita+ (2014) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.0216 | Huchra+ (1983) | rdg | MIS | 0 | Steep radio spectrum. Condon+ (2002) reported “very extended bent-tail radio source”. | ||
| J | 4C | 1.21 | Shaw+ (2012) | FSRQ | FSRQ | 0 | The first reported measurement of the redshift seems to be Baldwin+ (1978), but I cannot find the pdf on the web to confirm it. | ||
| J | 1RXS J | 0.177 | Table A2 | bll | UNCL | 1 | The 3FGL (Ackermann+ 2015) reported , but without any reference or information on the origin of this measurement. | ||
| J | CRATES J | 0.983 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.232 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.940 | Cohen+ (1987) | BLL | BLLAC | 0 | - | ||
| J | GB6 J | 0.595 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 1.27 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.976 | Schmidt (1977) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.157 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.536 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 0.455 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OD 166 | 2.68 | Afanas’ev+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 1.40 | Table A2 | bcu | UNCL | 1 | - | ||
| J | FIRST J | 0.409 | Becker+ (2001) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 1.80 | Baldwin+ (1981) | fsrq | FSRQ | 0 | - | ||
| J | S5 | 0.730 | Table A2 | bll | BLLAC | 1 | (Paiano+ 2017) | ||
| J | PKS | 0.635 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 351 | 0.265 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.985 | Paiano+ (2021) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.373 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B2 | 2.25 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.512 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.283 | Maza+ (1995) | fsrq | FSRQ | 0 | 6dF | ||
| J | PKS | 1.38 | Mahony+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.982 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.359 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RGB J | 0.243 | Archambault+ (2016) | bll | BLLAC | 0 | - | ||
| J | WN B | 0.625 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.37 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.42 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | B2 | 1.12 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | FBQS J | 0.535 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.537 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | MG3 J | 0.859 | Ricci+ (2015) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.580 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS B | 0.971 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 0.373 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.39 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | MG3 J | 0.484 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 1RXS J | 0.275 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.893 | Stickel+ (1989) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.545 | Caccianiga+ (2000) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.629 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.278 | Marchesini+ (2019) | bcu | BLLAC | 0 | - | ||
| J | PKS | 0.313 | Peña-Herazo+ (2021) | bcu | FSRQ | 0 | - | ||
| J | PKS | 0.823 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.481 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.451 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.196 | Fischer+ (1998) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.11 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.263 | Pesce+ (1995) | BLL | BLLAC | 0 | - | ||
| J | AT20G J | 0.829 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.35 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | RBS 385 | 0.597 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) | ||
| J | 4C | 0.475 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.511 | SDSS | bll | BLLAC | 0 | Brinkmann+ (2000) reported , but there are neither the spectrum nor any explanation on how this value was obtained. | ||
| J | PMN J | 0.880 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.312 | Paiano+ (2017) | bll | BLLAC | 0 | - | ||
| J | LEDA 095522 | 0.0289 | Wegner+ (1999) | bcu | BLLAC | 0 | - | ||
| J | 2MASS J | 0.170 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NGC 1218 | 0.0286 | Schmidt (1965) | rdg | MIS | 0 | Classified as LERG, FRI by Balmaverde+ (2021). S0 host galaxy. | ||
| J | PKS | 0.863 | Veron (1994) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.193 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | NVSS J | 0.199 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | PKS | 1.48 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.239 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 0.177 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.816 | Vermeulen+Taylor (1995) | fsrq | SEY | 0 | Redshift confirmed by SDSS. H narrow (FWHM Å km/s), flat radio spectrum, soft gamma-ray spectrum. There is an error in the Vizier version of Shaw+ (2012): the coordinates of B3 0307+380 are associated with the 1FGL J. | ||
| J | GALEXASC J | 0.380 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.558 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.399 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.664 | Strittmatter+ (1974) | fsrq | FSRQ | 0 | - | ||
| J | V Zw 326 | 0.0715 | Sargent (1970) | bll | BLLAC | 0 | - | ||
| J | B3 B | 0.134 | de Bruyn (1989) | rdg | MIS | 0 | Broad-Line Radio Galaxy, FRII (de Bruyn 1989). | ||
| J | TXS | 0.994 | Pursimo+ (2013) | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.143 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) classified it as BL Lac Object with with an uncertainty flag, but there are no information about this flag. | ||
| J | PMN J | 0.258 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.636 | Perlman+ (1998) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.57 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.435 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.372 | Stadnik+Romani (2014) | bll | BLLAC | 1 | - | ||
| J | RBS 405 | 0.443 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.210 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | IC 310 | 0.0190 | Arp (1968) | RDG | MIS | 0 | SDSS. Seyfert 1, SA0 host galaxy, large viewing angle, Homan+ (2021, subm). Detailed classification in Gendron-Marsolais+ (2020) | ||
| J | PMN J | 0.533 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.17 | Kapahi+ (1998) | fsrq | AMB | 0 | Kapahi+ (1998) also classified it as CSS on the basis of radio observations (), but the radio spectral index according to specfind is . Borderline object. | ||
| J | PKS | 0.0760 | Melnick+Quintana (1981) | bcu | MIS | 0 | In cluster, S0 host galaxy. Takizawa+ (2003) suggest it could be similar to M87 on the basis of X-ray observations with Chandra. Steep radio spectrum. | ||
| J | MG3 J | 1.83 | Table A2 | bll | UNCL | 1 | - | ||
| J | MRSS | 0.309 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1E | 0.190 | Gioia+ (1984) | bll | BLLAC | 0 | - | ||
| J | NGC 1275 | 0.0176 | Humason (1932) | RDG | MIS | 0 | Classified as FRI by Fanaroff+Riley (1974). | ||
| J | 1RXS J | 0.494 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.781 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.459 | Table A2 | bll | UNCL | 1 | - | ||
| J | MG3 J | 0.427 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | MG1 J | 1.34 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.031 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | 1H | 0.063 | Zhou+ (2007) | nlsy1 | NLS1 | 0 | Sb host galaxy. | ||
| J | PKS | 1.16 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 2MASX J | 0.128 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.0610 | Grazian+ (2002) | bll | BLLAC | 0 | - | ||
| J | RBS 421 | 0.291 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | TXS | 2.06 | Halpern+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.309 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1H | 0.147 | Filippenko+ (1986) | bll | BLLAC | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | CRATES J | 0.730 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | WISEA J | 0.345 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 0.719 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PGC 013066 | 0.0666 | Lucey+ (1983) | bcu | MIS | 0 | FR0 according to Glowacki+ (2017). | ||
| J | PMN J | 0.140 | Table A2 | bll | UNCL | 1 | - | ||
| J | SUMSS J | 0.277 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | 1RXS J | 0.207 | Álvarez Crespo+ (2016) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.934 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.807 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.863 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | - | - | bll | BLLAC | 2 | Álvarez Crespo+ (2016) | ||
| J | WN B | 0.791 | Table A2 | bll | UNCL | 1 | - | ||
| J | B3 | 0.392 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.068 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.36 | Shaw+ (2013) | bll | BLLAC | 0 | The first value of is reported by Barbieri+ (1975), referring to Burbidge+Strittmatter (1972), which in turn does not contain the source. The origin of that value of z cannot be found. Landoni+ (2015) found a featureless spectrum, likely due to a high activity of the jet. | ||
| J | 4C | 0.0206 | Peterson (1979) | rdg | MIS | 0 | Low-Power Compact radio galaxy (FR0?) according to Giovannini+ (2001). | ||
| J | SUMSS J | 0.163 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | NRAO 140 | 1.26 | Kristian+Sandage (1970) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.160 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.54 | Cristiani+Koehler (1987) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 3.45 | Chu+ (1986) | fsrq | FSRQ | 0 | - | ||
| J | 2E | 0.251 | Halpern+ (1997) | bll | BLLAC | 0 | - | ||
| J | RX J | 1.87 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | 1RXS J | 0.239 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | PKS | 0.0656 | Bauer+ (2000) | bll | MIS | 0 | FR0 according to Glowacki+ (2017). S0 host galaxy. | ||
| J | PKS | 0.852 | Bolton+Wall (1970) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.683 | Peña-Herazo+ (2017) | bcu | FSRQ | 0 | - | ||
| J | TXS | 0.618 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.223 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.945 | Shaw+ (2012) | fsrq | FSRQ | 0 | Warning: the source is in the machine-readable table on the published paper, but it was not ingested in the online table on Vizier. | ||
| J | PKS | 0.866 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.42 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.582 | Table A2 | bll | UNCL | 1 | - | ||
| J | OE 367 | 1.48 | Vermeulen+Taylor (1995) | fsrq | FSRQ | 0 | - | ||
| Jc | 1RXS J | - | - | bcu | UNCL | 3 | The young stellar cluster IC 348 is distant from the ROSAT counterpart (Preibisch+Zinnecker 2004). | ||
| J | 1RXS J | 0.251 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.526 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | PKS | 0.522 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.761 | Table A2 | bcu | UNCL | 1 | Fornax cluster, ? MIS? (Robertson+Roach 1990). | ||
| J | PKS | 0.991 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.39 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | AT20G J | 1.14 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.583 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1ES | 0.159 | Table A2 | bll | AMB | 1 | Schachter+ (1993) reported on the basis of weak absorption features of the host galaxy. There is another value of from a 6dF spectrum showing prominent emission lines identified as the H/[OIII] complex (Jones+ 2009, quality factor 4). Sbarufatti+ (2005) found an agreement between their imaging redshift and the Schachter’s one. Additionally, the SEDs published by several authors display the typical characteristics of a BL Lac object, which are inconsistent with the strong emission lines in the 6dF spectrum. A CLAGN? However, in this case, the first z would be wrong. | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 2.944 | Ellison+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.206 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.275 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.927 | Hook+ (2003) | bcu | FSRQ | 0 | - | ||
| J | GALEXASC J | 0.685 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.606 | Table A2 | bcu | UNCL | 1 | - | ||
| J | XRS J | 0.4 | Falomo+Ulrich (2000) | bll | BLLAC | 1 | - | ||
| J | PKS | 0.087 | Masetti+ (2006) | bll | MIS | 0 | Classified as FR0 by Glowacki+ (2017) (z wrong in that paper). | ||
| J | WN B | 0.0694 | Bauer+ (2000) | bll | BLLAC | 0 | Marchesi+ (2018) reported a featureless spectrum, likely due to a change in the jet activity. | ||
| J | S5 | 0.743 | Table A2 | bll | BLLAC | 1 | Henstock+ (1997) | ||
| J | PKS | 1.19 | Jauncey+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | CRATES J | 0.846 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.234 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.643 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | MG3 J | 1.25 | Table A2 | bcu | UNCL | 1 | Massaro+ (2015) reported , but with an uncertainty flag and no indication of the origin. Dallacasa+ (2000) classified it as GPS/HFP. | ||
| J | 2MASS J | 0.239 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.100 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | AT20G J | 0.488 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 0.654 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WN B | 0.662 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.136 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013). Arsioli+ (2015) gives , but with a uncertainty flag and no indication of the origin of this value. | ||
| J | PKS | 0.886 | Table A2 | bll | BLLAC | 1 | Drinkwater+ (1997) reported , but the published spectrum is almost featureless and there is no indication on which lines the value of z is based. Hook+ (2003) reported another featureless spectrum, and challenged the Drinkwater’s measurement. | ||
| J | GB6 J | 1.10 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.489 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 0.306 | Sowards-Emmerd+ (2005) | bcu | BLLAC | 0 | - | ||
| J | TXS | 0.834 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.626 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 1.27 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.407 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.29 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | OF 200 | 2.11 | Schmidt (1977) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.598 | Healey+ (2008) | bll | FSRQ | 0 | - | ||
| J | PKS | 1.42 | Surdej+Swings (1981) | FSRQ | FSRQ | 0 | - | ||
| J | PMN J | 0.554 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.22 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.571 | Lynds (1967) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.193 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | PKS | 1.28 | Veron+ (1990) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.13 | Sowards-Emmerd+ (2003) | bll | CLAGN | 0 | Classified as BL Lac Object by Sowards-Emmerd and reclassified as FSRQ by Shaw+ (2012). | ||
| J | NVSS J | 0.243 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.666 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | GB6 J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.833 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.02 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.735 | Table A2 | bcu | BLLAC | 1 | Paiano+ (2019) | ||
| J | RBS 526 | 0.825 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | 1RXS J | 0.698 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.475 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.385 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | SUMSS J | 1.04 | Table A2 | fsrq | UNCL | 1 | - | ||
| J | PKS | 1.54 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | 0.287 | Halpern+ (1991) | bll | BLLAC | 0 | - | ||
| J | PKS B | 0.125 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 1.26 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.14 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.257 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.225 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.193 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.242 | Shaw+ (2012) | fsrq | FSRQ | 0 | Shaw+ (2012) measured FWHM(H) = 2500 ± 800 km/s: candidate NLS1? | ||
| J | MS | 0.512 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | PKS | 2.28 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.649 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.915 | Bolton+ (1970) | FSRQ | FSRQ | 0 | - | ||
| J | PKS | 0.268 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.175 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015). The 3LAC indicated , but it seems to be the lower limit suggested by Shaw+ (2013), yet on the basis of a featureless spectrum. | ||
| J | 4C | 0.581 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.718 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.11 | Heidt+ (2004) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.33 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.06 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.10 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) | ||
| J | PKS | 1.42 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | 1.23 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MRSS | 0.218 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PMN J | 0.623 | Titov+ (2013) | bcu | FSRQ | 0 | - | ||
| J | MG1 J | 0.758 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.516 | Shaw+ (2012) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 1.35 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | TXS | 1.23 | Table A2 | bcu | BLLAC | 1 | Landt+ (2004, 2008) reported a featureless spectrum with a tentative based on absorption features (it would be a lower limit). | ||
| J | 3C 120 | 0.0336 | Arp (1968) | RDG | MIS | 0 | BLRG, Sy1, FRI, S0 host galaxy, Walker+ (1987) | ||
| J | NVSS J | - | - | bll | BLLAC | 2 | Paiano+ (2020) | ||
| J | 1RXS J | 0.217 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG2 J | 0.655 | Table A2 | bll | BLLAC | 1 | Many authors reported a featureless spectrum. However, Massaro+ (2009) gave with a uncertain flag and without information on the origin of this value. Paiano+ (2020) found a doubtful emission feature, which could be MgII (hence ). | ||
| J | PKS | 0.930 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.421 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | TXS | 0.928 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.979 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 0.882 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | 1RXS J | 0.418 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PKS | 0.8 | Table A2 | bcu | UNCL | 1 | - | ||
| J | AT20G J | 0.618 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.307 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | BLLAC | 2 | Peña-Herazo+ (2021) | ||
| J | PKS | 1.28 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.383 | Table A2 | bcu | AMB | 1 | Warning! The coordinates of the 4FGL proposed counterpart SUMSS J are (!) distant from the LAT centroid and well outside the 95% error contours (). NVSS J is the only radio source within the LAT centroid. Its optical spectrum from 6dF is inconclusive. | ||
| J | PKS | 2.02 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | IERS B | 1.27 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.343 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1SXPS J | 0.708 | Table A2 | bll | UNCL | 1 | - | ||
| J | RBS 570 | 0.324 | Table A2 | bll | BLLAC | 1 | Schwope+ (2000) set , but with uncertain flag. | ||
| J | PKS | 2.85 | Morton+ (1987) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 B | 0.2 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 1RXS J | 1.249 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.109 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.844 | Schmidt (1977) | fsrq | NLS1 | 0 | Shaw+ (2012) measured FWHM(H) = 1700 ± 1100. | ||
| J | GB6 J | 0.2 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.746 | Peña-Herazo+ (2021) | bcu | FSRQ | 0 | - | ||
| J | 1RXS J | 0.314 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) | ||
| J | PMN J | 0.844 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.097 | Abdo+ (2010) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.166 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MRC | 1.10 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 589 | 1.77 | Table A2 | bll | BLLAC | 1 | Chang+ (2017) | ||
| J | PKS | 2.15 | Shaw+ (2012) | fsrq | CLAGN | 0 | First value of is reported by von Montigny+ (1995), but with no indication of the origin. This value is challenged by Halpern+ (2003), who found a featureless spectrum (epoch 1996-2002). Additionally, Afanas’ev+ (2005) observed a featureless spectrum in 2001-2002. The spectrum taken by Shaw+ (2012) clearly shows a prominent CIV at (epoch unknown, but likely in 2010s). | ||
| J | S4 | 0.781 | Stickel+Kuhr (1993) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.205 | Perlman+ (1998) | bll | BLLAC | 0 | The first identification as FSRQ/Sy1 at by Craig & Fruscione (1997) is wrong. This source is distant from the radio position. The Perlman’s counterpart is almost coincident with the radio coordinates and the redshift value is confirmed by Prandini+ (2012). However, this value, based on the Ca H&K break, is not confirmed by Pita+ (2014), but the non-detection could be due to an increased jet activity. | ||
| J | PKS | 0.444 | Stickel+ (1989) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.742 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.552 | Table A2 | bcu | UNCL | 1 | - | ||
| J | AT20G J | 0.748 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.602 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.417 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 2.10 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 2.56 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.858 | Fricke+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.606 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.865 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | 4C | 0.405 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.01 | Stickel+ (1989) | FSRQ | BLLAC | 0 | - | ||
| J | NVSS J | 0.152 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.385 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.193 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 0.838 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S3 | 2.29 | Strittmatter+ (1974) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.11 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.35 | Truebenbach+Darling (2017) | bll | BLLAC | 0 | - | ||
| J | 1E | 0.240 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.04 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 2.26 | Table A2 | bll | BLLAC | 1 | Arsioli+ (2015) | ||
| J | PKS | 0.954 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | MG1 | 0.424 | Pita+ (2014) | bll | BLLAC | 0 | The value of by Bauer+ (2000) seems to be wrong. | ||
| J | TXS | 1.27 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.415 | Table A2 | bll | UNCL | 1 | - | ||
| J | S3 | 1.48 | Veron (1994) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.182 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.3 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) reported a featureless spectrum, with a hint of Ca H&K break, which would imply . | ||
| Jc | NVSS J | 1.22 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | 1WGA J | 0.486 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.593 | Table A2 | bcu | BLLAC | 1 | Paiano+ (2019) | ||
| J | 1ES | 0.101 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | 1RXS J | 0.288 | Table A2 | bcu | BLLAC | 1 | 6dF | ||
| J | PMN J | 1.09 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | 0.340 | Shaw+ (2013) | bll | BLLAC | 0 | There are two more estimates of z: one from Perlman (1998, ), reported by Scarpa+ (1999) as private communication; the other () is from Landt+ (2002), who challenged the Perlman’s measurement and proposed the new one after an inspection of the same spectrum. However, it was not possible to find these spectra either in publications or elsewhere. The only spectrum available online is that published by Shaw+ (2013). | ||
| J | PMN J | 1.88 | Álvarez Crespo+ (2016) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.577 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.336 | Paiano+ (2018) | bll | BLLAC | 0 | Neutrino blazar. | ||
| J | PKS | 0.621 | Shaw+ (2012) | fsrq | CLAGN | 0 | Afanas’ev+ (2005) observed a featureless spectrum: changing-look AGN. | ||
| J | S5 | 0.112 | Torrealba+ (2012) | bll | BLLAC | 0 | There is a long debate on the value of z. Lawrence+ (1996) suggested on the basis of a weak detection of [OIII]—confirmed by Torrealba+ (2012)—but Stocke+Rector (1997) suggested on the basis of an absorption feature identified as MgII. Warning: this lower limit is often confused as a measured value many times in the literature and by SIMBAD and NED. Scarpa+ (2000) supported the high-z lower limit on the basis of the host galaxy unresolved by HST. | ||
| J | 1H | 0.144 | Table A2 | bll | UNCL | 1 | There is a value available in the literature, but it was not possible to find either the origin of this measurement or a new spectrum confirming the value. The first paper found reporting this value is Laurent-Muehleisen+ (1993), but it has no reference. | ||
| J | RBS 625 | 0.271 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | PKS | 0.416 | Perlman+ (1998) | fsrq | CLAGN | 0 | Labiano+ (2007) reported by referring to de Vries+ (1997). However, the latter does not give any z for this source. On the contrary de Vries+ (2000) published a new spectrum confirming Perlman’s value, but with weaker lines and suggesting a BL Lac nature. This implies a changing-look AGN. Note that Shaw+ (2013) associated the gamma-ray source with another counterpart placed at from PKS and with a featureless spectrum. | ||
| J | CRATES J | 1.12 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | Warning: in the field of the Large Magellanic Cloud. | ||
| J | NVSS J | 0.793 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 0.167 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.16 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.194 | Stickel+ (1993) | fsrq | AMB | 0 | Stickel reported narrow H (FWHM∼2000 km/s): NLS1? SEY? FSRQ? | ||
| J | GB6 J | 0.648 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.536 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.251 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.30 | Shaw+ (2012) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.41 | Titov+ (2003) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.328 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.952 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.27 | Table A2 | bcu | UNCL | 1 | - | ||
| J | Pictor A | 0.0342 | Schmidt (1965) | rdg | MIS | 0 | FRII, BLRG, Seyfert 1, SA0 host galaxy Angioni+ (2020) | ||
| J | 3C 138 | 0.759 | Lynds+ (1966) | css | MIS | 0 | CSS, Seyfert 1.5, steep radio spectrum (borderline), details Dallacasa+ (2021) | ||
| J | TXS | 0.347 | Titov+ (2013) | fsrq | FSRQ | 0 | No line measurements, but the visual inspection of the spectrum shows prominent [OIII] lines, weak H, and FeII bumps. NLS1 or even SEY? | ||
| J | NVSS J | 1.54 | Table A2 | bll | BLLAC | 1 | The SDSS | ||
| J | PKS | 0.427 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.055 | Westerlund+Stokes (1966) | AGN | CLAGN | 0 | Changing-look AGN (Danziger et al. 1979, Ulrich 1981). Early optical spectroscopic observations (Westerlund+Stockes 1966) revealed an almost featureless spectrum, but with some weak features that allowed to measure z. More recent spectra displayed prominent emission lines typical of BLRG/Seyfert 1 galaxies (e.g., Stickel+ (1993), Sbarufatti+ (2006)). The radio morphology is FRI-type, with a viewing angle larger than 10 degrees (Angioni+ (2019)). | ||
| J | PMN J | 1.04 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.48 | Stickel+ (1993) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.092 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | SUMSS J | 0.637 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.704 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 1.30 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.30 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.2 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | PMN J | 0.0835 | Huchra+ (2012) | bcu | BLLAC | 0 | - | ||
| J | 1RXS J | 1.13 | Anderson+Filipovic (2009) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.240 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.784 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.685 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 2.07 | Hunter+ (1993) | FSRQ | FSRQ | 0 | - | ||
| J | PMN J | 0.812 | Titov+ (2017) | BLL | BLLAC | 0 | - | ||
| J | OG 50 | 1.25 | Sowards-Emmerd+ (2005) | FSRQ | FSRQ | 0 | - | ||
| J | PKS | 0.586 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.774 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | MRC A | 1.044 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.841 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.67 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.30 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.194 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.684 | Caccianiga+ (2000) | fsrq | FSRQ | 0 | 6dF | ||
| J | GALEXASC J | 0.619 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.130 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | NVSS J | 0.211 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | NVSS J | 1.124 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.894 | Peterson+ (1976) | BLL | BLLAC | 0 | - | ||
| Jc | TXS | 1.83 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 3.11 | Wright+ (1978) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | - | - | bll | BLLAC | 2 | Paiano+ (2020) | ||
| J | PKS | 1.19 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | In the field of LMC. | ||
| J | PKS | 0.839 | Stickel+Kuhr (1993) | fsrq | FSRQ | 0 | Chu+ (1986) suggested (uncertain) on the basis of one emission line identified as CIV. | ||
| J | PMN J | 0.201 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.273 | Pita+ (2014) | bll | BLLAC | 0 | - | ||
| Jc | NVSS J | 1.37 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.247 | Caccianiga+ (2002) | bll | BLLAC | 0 | Arsioli+ (2015) reported , but there is no indication on the origin of this measurement. | ||
| J | PMN J | 0.283 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.00 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.0689 | Fosbury+Disney (1976) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.956 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.332 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.605 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.07 | Table A2 | bll | UNCL | 1 | - | ||
| Jc | PMN J | 1.92 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | - | - | bcu | UNCL | 3 | - | ||
| J | SUMSS J | 0.467 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | 1RXS J | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.718 | Table A2 | bcu | UNCL | 1 | - | ||
| J | EXO | 0.302 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.557 | Table A2 | bcu | UNCL | 1 | McCarthy+ (1996) suggested a radio galaxy classification. | ||
| J | PKS | 0.194 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 0.318 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.66 | Perlman+ (1998) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 2.41 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.0524 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.134 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 1.22 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.0522 | Paiano+ (2020) | bcu | BLLAC | 0 | - | ||
| J | PMN J | 0.118 | de Menezes+ (2020) | bcu | BLLAC | 0 | - | ||
| J | SUMSS J | 0.203 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1ES | 0.130 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | SUMSS J | 0.760 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 1.14 | Vermeulen+Taylor (1995) | bcu | FSRQ | 0 | - | ||
| J | GB6 J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.0298 | Pietsch+ (1998) | bcu | SEY | 0 | Pietsch classified it as Seyfert2/LINER. | ||
| J | CRATES J | 0.682 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.275 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.02 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | S4 | 1.97 | Fomalont+ (2000) | fsrq | FSRQ | 0 | The redshift comes from a personal communication by Vermeulen & Taylor. No spectrum published. | ||
| J | PKS | 0.871 | Allington-Smith+ (1991) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.09 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.10 | Landoni+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.00 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.92 | Spinrad+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.710 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | PMN J | 0.485 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.77 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 7C | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 1.063 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.873 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.403 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.764 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | GB6 J | 0.812 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.289 | Table A2 | bll | BLLAC | 1 | Hook+ (2003) | ||
| J | 1RXS J | - | - | bll | UNCL | 3 | - | ||
| J | PMN J | 1.08 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.592 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | IVS B | 0.098 | Shaw+ (2013) | bll | BLLAC | 0 | There is another value – —reported in the 1FGL, but without any information except for a forthcoming paper (Piranomonte+D’Elia 2010, in preparation) that was never published. | ||
| J | PMN J | 0.299 | Álvarez Crespo+ (2016) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.29 | Table A2 | bcu | UNCL | 1 | NED reports from Liang+Liu (2003). However, that paper did not deal with the optical identification: there is just an acknowledgement to G. Z. Xie for optical observations. No other more recent observation has been published to confirm this value of redshift. | ||
| J | PKS | 1.90 | Ellison+ (2004) | bcu | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | IVS B | 1.21 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | 1RXS J | 0.529 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.414 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | RX J | 0.129 | Keel+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | MS | 0.513 | Landoni+ (2013) | bll | BLLAC | 1 | Landoni reported in his Table 2, but also in his Figure 6. Upon request, Landoni confirmed . However, the value remains uncertain because the spectrum is featureless and z is calculated with reference to a zero-velocity template. | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 0.591 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | PMN J | 2.05 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.775 | Table A2 | bll | UNCL | 1 | - | ||
| J | 2MASS J | 0.3 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.0546 | Tadhunter+ (1993) | rgd | MIS | 0 | FRI, Ekers+ (1989) | ||
| J | GB6 J | 0.131 | Table A2 | bcu | UNCL | 1 | SIMBAD gives likely from Jannuzi+ (1998), but that optical source HS is about far from the radio position. Therefore, the association is likely to be wrong. | ||
| J | PKS | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | PKS | 1.72 | Shaw+ (2013) | bll | BLLAC | 0 | Tentative, one weak emission line (CIV). | ||
| J | NVSS J | 0.717 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.23 | Table A2 | bll | BLLAC | 1 | Landt (2012). Warning: Landt+Bignall (2008) reported as certain, while Landt (2012) wrote that it is a lower limit, because it is based on a MgII absorption doublet. | ||
| J | PMN J | 1.51 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.53 | Ackermann+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.659 | Monroe+ (2016) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 1.17 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISE J | 0.478 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.386 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S5 | 1.85 | Stickel+Kuhr (1996) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.704 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.772 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.93 | Klindt+ (2017) | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.234 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017). SIMBAD proposes from Sowards-Emmerd+ (2005), but this paper does not have this source in its list. | ||
| J | NVSS J | 0.784 | Table A2 | bcu | BLLAC | 1 | 6dF | ||
| J | PKS | 0.681 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | 0.161 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | BLLAC | 2 | Shaw+ (2013) | ||
| J | B3 | 0.577 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.15 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.233 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | NVSS J | - | - | bll | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1ES | 0.41 | Kotilainen+ (2011) | bll | BLLAC | 1 | A first tentative estimate of by Falomo+Kotilainen (1999) is still often adopted, but seems to be wrong. The current redshift is estimated from the imaging of the host galaxy and is consistent with Meisner+Romani (2010). The most recent high S/N observation by Paiano+ (2017) still resulted in no features. | ||
| J | RX J | 0.316 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | NVSS J | 0.600 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WN B | 0.793 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.4 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | GB6 J | 0.891 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | LEDA 571171 | 0.091 | Mahony+ (2011) | bcu | MIS | 0 | FRI according to Glowaki+ (2017). The 6dF redshift by Jones+ (2009) is wrong, likely due to a contaminating star. | ||
| J | GB6 J | 1.25 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 0.933 | Henstock+ (1997) | FSRQ | FSRQ | 0 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | B3 | 0.126 | Marcha+ (1996) | bll | BLLAC | 0 | - | ||
| J | 4C | 0.059 | Laurent-Muheleisen+ (1998) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.421 | Titov+ (2013) | bcu | FSRQ | 0 | - | ||
| J | B2 A | 1.21 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.73 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.424 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.592 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | 1RXS J | 0.602 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.822 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | - | - | bll | UNCL | 3 | - | ||
| J | B3 | 0.613 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.618 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 0.626 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.656 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | NVSS J | 0.565 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 0.327 | Table A2 | bll | BLLAC | 1 | Henstock+ (1997) | ||
| J | NGC 2329 | 0.0192 | Peterson (1979) | rdg | MIS | 0 | FRI, Wide-Angle Tail, S0 host galaxy, Ferretti+ (1985). | ||
| J | GB6 J | 0.297 | Paiano+ (2020) | bll | BLLAC | 0 | - | ||
| J | 1H | 0.125 | Giommi+ (1991) | bll | BLLAC | 0 | - | ||
| J | AT20G J | 0.129 | Nkundabakura+Meintjes (2012) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 1.29 | Stickel+Kuhr (1994) | bll | FSRQ | 0 | - | ||
| J | RX J | 0.095 | Beckmann+ (2003) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.502 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.600 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.540 | Shaw+ (2009) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 1.00 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | SUMSS J | 0.175 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | S4 | 0.943 | Stickel+Kühr (1994) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | 1RXS J | 0.339 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | B2 | 0.779 | White+ (2000) | fsrq | CLAGN | 0 | Likely a changing-look AGN, because early observations reported a featureless spectrum (Wills+ (1986)). | ||
| J | 1RXS J | 0.223 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | PMN J | 1.25 | Titov+ (2013) | bcu | FSRQ | 0 | There is a discrepancy between SIMBAD and NED coordinates (the two positions are distant each other). The source corresponding to the coordinates given in the 4FGL is that of NED. | ||
| J | S5 | 0.31 | Nilsson+ (2008) | BLL | BLLAC | 1 | - | ||
| J | MG2 J | 0.786 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.232 | Table A2 | bll | UNCL | 1 | Appenzeller+ (1998) reported a blue galaxy coincident with the radio counterpart and suggest it could be a BL Lac Object, but there are no indication of any optical spectrum. | ||
| J | GB6 J | 0.966 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.555 | Table A2 | bcu | BLLAC | 1 | Marchesini+ (2019) | ||
| J | 4C | 1.04 | Healey+ (2008) | FSRQ | FSRQ | 0 | - | ||
| J | WN B | 0.119 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.69 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | SDSS J | 0.791 | Landoni+ (2018) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.963 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.186 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | GB6 J | 0.745 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.424 | Vermeulen+Taylor (1995) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.112 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.106 | Klindt+ (2017) | bll | BLLAC | 0 | - | ||
| J | RGB J | 0.248 | Wei+ (1999) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.457 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.668 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.756 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.0650 | Becerra González+ (2020) | bcu | BLLAC | 0 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 1.24 | Djorgovski+ (2010) | bcu | BLLAC | 0 | - | ||
| Jc | 4C | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 0.599 | Table A2 | bll | AMB | 1 | Although there is a SDSS spectrum available, the weak features do not allow to clearly measure the redshift. SDSS gives , but Mishra+ (2018), on the basis of the same spectrum, indicate , while Massaro+ (2009) give (but, in this case, the origin of this value is not evident). A better, conclusive spectrum is not available. | ||
| J | GB6 J | 3.01 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.720 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | SUMSS J | 0.2 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.45 | Nilsson+ (2012) | bll | BLLAC | 1 | It is often found in the literature the value of , but this is a lower limit due to the detection of absorption lines (MgII) by Carswell+ (1974). | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.191 | Lynds (1967) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.5 | Table A2 | bcu | UNCL | 1 | - | ||
| J | LEDA 1979979 | 0.179 | SDSS | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.946 | Smith+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.765 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 2.31 | Jorgenson+ (2006) | fsrq | FSRQ | 0 | SDSS | ||
| J | GB6 J | 0.723 | Halpern+Eracleous (1997) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 2.32 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.579 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| Jc | MRC | - | - | bcu | UNCL | 3 | - | ||
| J | MS | 0.315 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | PKS | - | - | bcu | BLLAC | 2 | Peña-Herazo+ (2021) | ||
| J | PKS | 0.994 | White+ (1988) | fsrq | FSRQ | 0 | Fricke+ (1983) reported a featureless spectrum, thus classifying it as BL Lac Object. However, the position is about distant from the radio position. The SDSS image shows three close sources, and Fricke’s source is the Southern one. White’s position is consistent with PKS coordinates. | ||
| J | 2MASS J | 0.621 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 2.99 | Sambruna+ (2006) | fsrq | FSRQ | 0 | Extreme MeV blazar. SDSS | ||
| J | OI 272 | 0.793 | Table A2 | fsrq | BLLAC | 1 | SDSS | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Ricci+ (2015) | ||
| J | RX J | 0.194 | Table A2 | bll | BLLAC | 1 | Bauer+ (2000) | ||
| J | 2MASS J | 0.405 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.748 | Table A2 | bcu | BLLAC | 1 | Marchesini+ (2019) | ||
| J | NVSS J | 0.246 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OI 275 | 0.410 | Stickel+ (1989) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.174 | Brinkmann+ (2000) | bll | BLLAC | 0 | SDSS. Interestingly, Massaro+ (2015) reported a featureless spectrum, likely due to an increased jet activity. | ||
| J | SDSS J | 0.559 | SDSS | bcu | FSRQ | 0 | - | ||
| J | TXS | 0.214 | Afanas’ev+ (2005) | bcu | BLLAC | 0 | - | ||
| J | SDSS J | 0.859 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.605 | Beckmann+ (2003) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.16 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | OI 280 | 0.889 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | JVAS J | 0.543 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.275 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG2 J | 0.699 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.269 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OI 380 | 1.94 | Schmidt (1977) | fsrq | FSRQ | 0 | SDSS | ||
| J | 4C | 0.73 | Sbarufatti+ (2005) | bll | BLLAC | 1 | SIMBAD, NED, and other papers reported from Stickel+Kuhr (1993), but this is a lower limit, not a measured value. The most recent spectroscopic observation by Shaw+ (2013) still found no emission lines. | ||
| J | TXS | 0.923 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.733 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB1 | 0.736 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | SUMSS J | 0.296 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.266 | Carangelo+ (2003) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.569 | Afanas’ev+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NGC 2484 | 0.041 | Colla+ (1975) | rdg | MIS | 0 | SDSS, FRI/LERG, S0 host galaxy, Owen+Laing (1989) | ||
| J | SDSS J | 0.099 | SDSS | bll | BLLAC | 0 | - | ||
| J | SDSS J | 0.693 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.621 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.682 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.685 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RX J | 0.188 | Table A2 | bll | BLLAC | 1 | A tentative was proposed by Caccianiga+ (2002). | ||
| J | GB6 J | 0.681 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bll | BLLAC | 2 | Paiano+ (2017) reported a featureless spectrum, but the coordinates of the observed object are different from those of 4FGL (∼). Both SDSS (only photometry, classified as a star) and LAMOST reported an optical source at from the 4FGL coordinates. LAMOST spectrum suggests a BLLAC at (H-[NII] complex at Å and Ca H+K break at Å). | ||
| J | WISEA J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.722 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.542 | Table A2 | fsrq | UNCL | 1 | Chang+ (2019) reported and a BLLAC classification, but it is not clear the origin of this value. Spectroscopic redshift should come from SDSS, but nothing is available on the online archive. | ||
| J | GB6 B | 2.67 | SDSS | bcu | FSRQ | 0 | - | ||
| J | TXS | 0.482 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.740 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WN B | 1.57 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 1.39 | Healey+ (2008) | fsrq | FSRQ | 0 | Jackson+ (2002) give on the basis of the association with the cluster Zw . However, the radio positions differ by . | ||
| J | TXS | 3.03 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.121 | Nass+ (1996) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.576 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | CRATES J | 0.865 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 2.11 | Henstock+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | SBS | 0.3 | Nilsson+ (2003) | bll | BLLAC | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.837 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | 0.481 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 1.10 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.84 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | OJ 508 | 1.43 | Hewitt+Burbidge (1987) | fsrq | FSRQ | 0 | Confirmed by SDSS. There are two more values, obviously wrong: from Arp+ (1990) and from Zieba+Chyzy (1991). | ||
| J | S4 | 1.42 | Xu+ (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | 87GB | 2.14 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 | 0.082 | Marcha+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | 1ES | 0.138 | Bade+ (1998) | BLL | BLLAC | 0 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Ackermann+ (2016) give , but this is a lower limit from absorption features in the spectrum, as indicated by Shaw+ (2013). | ||
| J | OJ 014 | 1.15 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.173 | Paiano+ (2020) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.463 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MG1 J | 0.908 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.909 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.170 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | NVSS J | 0.288 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.256 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.767 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | RX J | 0.374 | SDSS | bll | FSRQ | 0 | - | ||
| J | 1RXS J | 0.630 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.239 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | OJ 230 | 1.03 | Mavrides+Mutus (1984) | fsrq | FSRQ | 0 | SDSS | ||
| J | 2MASX J | 0.331 | Brand+ (2005) | bcu | BLLAC | 0 | SDSS. The source is in a sample of radio galaxies, but there is no indication of what type, and the radio spectrum is flat (). | ||
| J | NVSS J | 0.371 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SBS | 0.404 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Paiano+ (2020) | ||
| J | SDSS J | 0.867 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.611 | Table A2 | bcu | AMB | 1 | The 4FGL indicated as counterpart the radio source CRATES J, which in turn does not match the coordinates (difference ). Another radio source matches the coordinates, and we considered it as the counterpart. Glikman+ (2007) reported , and also indicated a Sb morphology of the host galaxy. However, Glickman+ (2012) reported for the same source and an identification with a starburst galaxy. The SDSS spectrum matching the 4FGL coordinates displays an evident emission line at Å, but the identification with Ly seems unlikely. If it is [OIII], then and the absorption at Å might be the Ca H+K. | ||
| J | RX J | 0.752 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.71 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | S4 | 0.61 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 0.225 | SDSS | bll | BLLAC | 0 | - | ||
| J | B2 | 0.671 | Table A2 | bll | BLLAC | 1 | SDSS gives on the basis of one feature identified as H. However, the spectrum is quite noisy and the identification rather doubtful. | ||
| J | RX J | 0.651 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS gives , but it likely a wrong identification due to the low S/N. | ||
| J | 5C | 0.578 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 0.389 | SDSS | bll | BLLAC | 0 | Véron-Cetty+Véron (2006) give the same value of z, but with reference to White+ (2000), which in turn do not report any z and commented with “uncertain quasar classification”. | ||
| J | RX J | 0.299 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | MG2 J | 0.447 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.402 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.539 | Landoni+ (2013) | bll | BLLAC | 0 | There are several values of z, likely due to the weakness of the emission features. Landoni+ (2013) reported FWHM(H) = 1100 km/s, but this is likely due to the weakness of the emission line ( Å) caused by a high jet activity (see Foschini 2012), rather than a NLS1 nature. | ||
| J | SDSS J | 0.954 | SDSS | bcu | FSRQ | 0 | - | ||
| J | B3 | 0.865 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.202 | Table A2 | bll | UNCL | 1 | - | ||
| J | OJ 233 | 0.951 | Stickel+ (1991) | bll | BLLAC | 0 | SDSS | ||
| J | B2 | 1.24 | Willot+ (1998) | fsrq | FSRQ | 0 | - | ||
| J | OJ 535 | 1.42 | Wills+Wills (1976) | fsrq | FSRQ | 0 | SDSS | ||
| J | 4C | 1.22 | Schmidt (1974) | fsrq | FSRQ | 0 | Please note that ADS has scanned the first printing of the Schmidt’s paper, which do not include the table with the redshifts because of an error, but not the Errata Corrige, where the table is printed. It was necessary to retrieve the correct paper from our local library. There are also data from SDSS. | ||
| J | PKS | 0.506 | Stickel+ (1991) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.204 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 0.120 | Table A2 | bll | BLLAC | 1 | 6dF. Massaro+ (2013) reported , but the origin is unknown. They cited 6dF, which in turn is featureless (, quality factor 1). Another value of is given by 3FGL (Ackermann+ (2015)), but—again—the origin is unknown. In addition, 3FGL classified this source as bcu, which should be unlikely once you have the optical spectrum. | ||
| J | TXS | 0.338 | Hook+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.24 | Brand+ (2005) | bll | BLLAC | 1 | - | ||
| J | B3 | 0.226 | Wei+ (1999) | bll | BLLAC | 0 | SDSS. Steep radio spectrum: MIS? | ||
| J | NVSS J | 0.415 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.0894 | Bauer+ (2000) | bll | MIS | 0 | SDSS. Miraghei+Best (2017) indicated a FRI morphology. | ||
| J | TXS | 0.866 | Landt+ (2001) | fsrq | MIS | 0 | Landt+ (2001) indicated a steep radio spectrum, confirmed also by specfind, and classified is as SSRQ. | ||
| J | NVSS J | 0.386 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.206 | SDSS | bcu | BLLAC | 0 | - | ||
| J | 1RXS J | 0.5 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S3 | 0.941 | Steidel+Sargent (1991) | FSRQ | FSRQ | 0 | SDSS | ||
| J | MG2 J | 1.05 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.539 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.174 | Falomo (1991) | bll | BLLAC | 0 | SDSS | ||
| J | OJ 250 | 0.255 | Table A2 | bcu | UNCL | 1 | Wills+Wills (1976) indicated a M-type star, but no spectrum published. No other spectra have been published. | ||
| J | OJ 448 | 0.548 | Stickel+ (1993) | bll | BLLAC | 0 | - | ||
| J | PMN J | 3.45 | Paliya+ (2020) | fsrq | FSRQ | 0 | - | ||
| J | OJ 451 | 0.249 | Henstock+ (1997) | fsrq | CLAGN | 0 | SDSS shows evident emission lines. On the opposite, LAMOST spectra are quite noisy, but the H seems to be confirmed, although much weaker than SDSS spectrum (1, 2, 3). Likely a changing-look AGN: also Hook+ (1996) found a noisy and featureless spectrum before Henstock. | ||
| J | B3 | 0.518 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 1.63 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.06 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.544 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MG2 J | 0.776 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.75 | Fricke+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | RGB J | 0.278 | SDSS | bll | BLLAC | 0 | - | ||
| J | TXS | 0.28 | Abraham+ (1991) | bll | BLLAC | 1 | - | ||
| J | NVSS J | 0.546 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.12 | Owen+ (1995) | fsrq | FSRQ | 0 | - | ||
| J | 3C 207 | 0.680 | Lynds (1967) | ssrq | MIS | 0 | FRII, HERG, steep radio spectrum Laing+ (1983). SDSS. | ||
| J | 4C | 2.17 | Stickel+ (1989) | FSRQ | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.425 | SDSS | bll | BLLAC | 0 | The SDSS spectrum is rather noisy, but the redshift was confirmed by observations at NTT by Kügler+ (2014). | ||
| J | TXS | 0.121 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.21 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.360 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | MG1 J | 0.597 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | WISE J | 1.22 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.059 | Shaw+ (2013) | bcu | BLLAC | 0 | - | ||
| J | RX J | 0.198 | Cao+ (1999) | bll | BLLAC | 0 | SDSS | ||
| J | TXS | 0.440 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.24 | Wright+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | SDSS J | 0.305 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | GB6 J | 0.810 | Table A2 | bcu | BLLAC | 1 | Paiano+ (2019) | ||
| J | PMN J | 0.636 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.094 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | TXS | 0.531 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 0.442 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SBS | 0.584 | Zhou+ (2005) | NLSY1 | NLS1 | 0 | SDSS | ||
| J | PMN J | 0.566 | Halpern+Eracleous (1997) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.145 | Brinkmann+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | GB6 J | 0.569 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B2 | 1.29 | Stocke+ (1983) | fsrq | FSRQ | 0 | SDSS | ||
| J | SDSS J | 0.494 | SDSS | bll | BLLAC | 0 | - | ||
| J | B3 | 0.093 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | OJ 287 | 0.306 | Miller+ (1978) | BLL | BLLAC | 0 | Miller’s value (tentative) was later confirmed by Sitko+Junkkarinen (1985) during an observation with the jet in low state. | ||
| J | PKS | 0.827 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.541 | Pursimo+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.20 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 0.376 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.679 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.281 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.660 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | 3C 212 | 1.05 | SDSS | ssrq | MIS | 0 | FRII according to Laing+ (1983). | ||
| J | 1RXS J | 0.920 | SDSS | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.327 | Beckmann+ (2003) | bll | BLLAC | 0 | - | ||
| J | AT20G J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.478 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.970 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | NVSS J | 0.288 | SDSS | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.566 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.56 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 1.16 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | S4 | 1.46 | Lawrence+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 | 1.72 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 4C | 1.34 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | MG1 J | 0.224 | Paiano+ (2020) | bll | BLLAC | 0 | - | ||
| J | CRATES J | 0.412 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.863 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 87GB | 1.64 | Glikman+ (2004) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.432 | Rosa-González+ (2017) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.02 | Burbidge+Strittmatter (1972) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 1.75 | Ching+ (2017) | bll | BLLAC | 0 | - | ||
| J | B2 | 0.272 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.957 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | - | ||
| J | 3C 216 | 0.670 | Smith+Spinrad (1980) | css | CLAGN | 0 | CSS/HERG, see Barthel+ (1988) and Best+Heckman (2012). Schmidt (1968) reported a featureless spectrum, implying a changing-look AGN. SDSS, LAMOST. | ||
| J | TXS | 2.68 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | Ton 1015 | 0.608 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020). Please note an error in the CDS catalog of Bauer+ (2000), which affected also the entries in SIMBAD and NED databases: it is written , but the note reported a featureless spectrum. | ||
| J | FBQS J | 0.199 | SDSS | bll | BLLAC | 0 | - | ||
| J | MG2 J | 0.456 | SDSS | bll | BLLAC | 0 | - | ||
| J | RX J | 0.903 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | B3 B | 2.57 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 1.75 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.212 | Bauer+ (2000) | bll | BLLAC | 0 | Warning: the 4FGL indicated RX J as counterpart, but this X-ray source is usually associated with the cluster Abell 763 (). The closest radio source and the most likely counterpart is NVSS J (distant from the 4FGL coordinates), which is a background BL Lac not associated with the cluster. | ||
| J | MRC | 0.198 | Jones+ (2009) | bll | BLLAC | 0 | Although the quality flag of the 6dF spectrum is 3 (reliable %), the Ca H&K break is clearly visible. | ||
| J | 1RXS J | 0.639 | Beckmann+ (2003) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.519 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.427 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | Ton 396 | 0.035 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | 4C | 1.268 | Allington-Smith+ (1988) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.190 | Nass+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.847 | Wright+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.308 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.783 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.491 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.896 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 2.188 | Hewitt+Burbidge (1987) | fsrq | FSRQ | 0 | SDSS. Complex radio morphology (core+lobe, jet bending , Neff+Hutchings (1990)), but flat radio spectrum and superluminal motion () according to the MOJAVE project. | ||
| J | NVSS J | 0.181 | Table A2 | bll | UNCL | 1 | - | ||
| J | OK 630 | 1.447 | Stickel+Kühr (1993) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.555 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.974 | Healey+ (2008) | fsrq | AMB | 0 | Healey+ (2008) classified it as NLRG, because of FWHM km/s (no images of the optical spectrum are available), but the radio spectrum is flat (from NED, ). Perhaps SEY? | ||
| J | GB6 J | 0.656 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.457 | SDSS | bcu | SEY | 0 | Deller+Middleberg (2014) reported a compact radio source. Radio spectrum is flat. | ||
| J | B2 | 0.79 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 1.73 | Shaw+ (2012) | fsrq | FSRQ | 0 | Some differences in redshift measurements: the first observation (Hook+ 1996) resulted in a featureless spectrum; then, Falco+ (1998) reported a galaxy-dominated spectrum at , on the basis of H and [OIII] (plus weak H and Ca H&K), but there was no spectrum published. The SDSS spectrum is quite noisy, but similar to that published by Shaw+ (2012). The featureless spectrum reported by Hook+ (1996) seems to be due to low S/N rather than a real change of classification. | ||
| J | RBS 771 | 0.432 | Table A2 | bll | BLLAC | 1 | SDSS and LAMOST inconclusive. Piranomonte+ (2007) reported a featureless spectrum and set . Chang+ (2019) reported a firm redshift of , but no spectrum was published. It seems the value of the automatic pipeline of SDSS DR3, which is unreliable because the spectrum is featureless and noisy. | ||
| J | B2 | 0.744 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | B2 B | 0.26 | Tinti+de Zotti (2006) | bll | BLLAC | 1 | - | ||
| J | NVSS J | 1.18 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.608 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MG2 J | 0.649 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 0.347 | Peterson+ (1979) | fsrq | FSRQ | 0 | 6dF | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | PKS B | 0.733 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.747 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | - | - | bll | UNCL | 3 | - | ||
| J | GB6 J | 0.339 | Table A2 | bll | BLLAC | 1 | SDSS. A value of is often found in the literature, but it is one of the early measurement from the SDSS DR3: unreliable. | ||
| J | NVSS J | 0.208 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | SDSS J | 0.439 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S5 | 1.35 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 1ES | 0.187 | Perlman+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | B2 | 0.977 | Table A2 | bll | BLLAC | 1 | Caccianiga+ (2002) | ||
| J | PKS | 1.77 | SDSS | fsrq | FSRQ | 0 | Early estimation was by Jauncey+ (1984), who identified a line at 4211 Å as MgII. The SDSS spectrum shows that instead it is CIV. Other lines in the spectrum support this finding. | ||
| J | TXS | 0.536 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.205 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.660 | SDSS | rdg | BLLAC | 0 | 4FGL associated this source to the radio galaxy NGC 2892, which is distant from the coordinates of the proposed counterpart. We considered valid the RA and Dec of the counterpart, corresponding to the SDSS source. | ||
| J | S4 | 0.597 | Stickel+Kuhr (1994) | fsrq | NLS1 | 0 | FWHM(H) km/s (Rakshit+ (2017)). SDSS | ||
| J | NVSS J | 0.361 | SDSS | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.748 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RXC J | 0.250 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.340 | Table A2 | bll | BLLAC | 1 | Desai+ 2019 | ||
| J | TXS | 0.699 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 0.561 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.276 | Henstock+ (1997) | fsrq | SEY | 0 | SDSS. Rakshit+ (2017) classified it as NLS1, with FWHM(H) km/s and weak FeII. However, Henstock+ (1997) reported FWHM(H) km/s, and also Shaw+ (2012) measured a broad FWHM(H) km/s on the same SDSS spectrum. The H profile is distorted at its base and there is significant noise. It seems more an intermediate Seyfert. | ||
| J | NVSS J | 0.287 | Paiano+ (2017) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.831 | Krogager+ (2018) | bcu | FSRQ | 0 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.211 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | TXS | 0.551 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.816 | White+ (2000) | bcu | FSRQ | 0 | SDSS | ||
| J | GB6 J | 0.546 | Table A2 | bll | BLLAC | 1 | In the 2LAC the source is identified as fsrq with , but in the more recent version of the catalog, the source is identified as bll without redshift. SDSS spectrum is inconclusive, but at least it favors a BLLAC identification. | ||
| J | NVSS J | 0.366 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.531 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ 2016 | ||
| J | FIRST J | 0.791 | SDSS | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.423 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | WISE J | 0.563 | Walsh+ (1984) | fsrq | FSRQ | 0 | SDSS | ||
| J | B3 | 0.639 | Britzen+ (2007) | fsrq | MIS | 0 | SDSS. Healey+ (2008) also performed optical spectroscopy and confirmed the value of z, but they classified it as fsrq. Britzen+ (2007) have also analyzed radio data (VLA), which allowed them to estimate the viewing angle and . | ||
| J | GB6 J | 0.229 | SDSS | bll | BLLAC | 0 | SDSS shows another object with the same redshift at (∼19 kpc), but with a redder spectrum and no radio counterpart. No specific publication was found in the literature. Interacting galaxies? | ||
| J | RX J | 0.575 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.577 | SDSS | bll | BLLAC | 0 | - | ||
| J | TXS | 1.004 | Afanas’ev+ (2003) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | - | - | bll | UNCL | 3 | - | ||
| J | TXS | 0.498 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.187 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.882 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.584 | Williams+ (2002) | NLSY1 | NLS1 | 0 | SDSS | ||
| J | 4C | 1.25 | Wills+Wills (1976) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.693 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | 87GB | 1.42 | SDSS | bcu | FSRQ | 0 | - | ||
| J | GB6 J | 0.615 | Table A2 | bll | BLLAC | 1 | SDSS inconclusive. Ching+ (2017) reported an uncertain from Drinkwater+ (2010), which in turn does not contain the source. | ||
| J | RX J | 0.409 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RX J | 0.777 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RBS 804 | 0.181 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | SDSS J | 0.574 | Paiano+ (2017) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.743 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | RX J | 0.109 | Peña-Herazo+ (2021) | bcu | BLLAC | 0 | - | ||
| J | 1ES | 0.207 | Morris+ (1991) | bll | BLLAC | 1 | - | ||
| J | 1RXS J | 0.557 | Paiano+ (2020) | bll | BLLAC | 0 | Possible neutrino source. | ||
| J | NVSS J | 0.630 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | WISE J | 1.173 | Vigotti+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.161 | Grazian+ (2002) | bll | BLLAC | 0 | - | ||
| J | OK 290 | 0.708 | Burbidge+Strittmatter (1972) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 1.32 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 4C | 0.903 | Wills+Wills (1974) | fsrq | FSRQ | 0 | SDSS. Double peaked H and other lines with evident red wings. | ||
| J | B2 | 0.279 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | 3C 232 | 0.531 | Wills (1966) | fsrq | NLS1 | 0 | SDSS. Phillips (1978) reported the typical NLS1 spectrum (FWHM(H) km/s, bump FeII), but at that epoch the classification was not yet invented. Boksenberg+Sargent (1978) reported Ca H&K absorption features in the spectrum of 3C 232, which are due to the nearby (∼) spiral galaxy NGC 3067. | ||
| J | OK 492 | 1.88 | Burbidge+ (1977) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.554 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007) | ||
| J | 1RXS J | 0.174 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NGC 3078 | 0.00828 | Humason+ (1956) | rdg | AMB | 0 | Compact radio core, flat radio spectrum. It is indicated as radiogalaxy in the 4FGL, but the radio properties are not those of a radiogalaxy. No optical spectrum was published. | ||
| J | 7C | 1.15 | Hook+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.986 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 0.368 | Lawrence+ (1986) | BLL | BLLAC | 0 | - | ||
| J | GB6 J | 0.239 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.365 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | 2MASX J | 0.148 | Peña-Herazo+ (2021) | bcu | SEY | 0 | SDSS displays only photometry and the image shows a likely edge-on spiral galaxy. The optical spectrum shows strong H, [OIII], and [OII] emission lines. Perhaps MIS? | ||
| J | GB6 J | 0.556 | Shaw+ (2012) | bll | FSRQ | 0 | The SDSS spectrum displays an evident emission line at Å, which was incorrectly identified as [OIII], resulting in a zero-value redshift. | ||
| J | 1RXS J | 0.616 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SDSS J | 0.786 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 0.606 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.149 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.732 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.330 | Bolton+Savage (1977) | fsrq | FSRQ | 0 | - | ||
| J | EXO | 0.640 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.84 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.0977 | Grandi (1983) | bcu | MIS | 0 | Classified as FRI by Owen+ (1995) (redshift refinement and emission line properties) and Owen+ (1996) (radio morphology). Yuan+ (2016) reported , but it is not clear the origin of this measurement. | ||
| J | MG1 J | 1.72 | Urrutia+ (2009) | bll | BLLAC | 0 | Shaw+ (2013) found a featureless spectrum, likely due to a change in the jet activity. | ||
| J | RX J | 0.343 | Bade+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 1.67 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.534 | Landoni+ (2020) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.143 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.887 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | 2dF | ||
| J | PKS B | 1.59 | Perlman+ (1998) | fsrq | FSRQ | 0 | - | ||
| J | NRAO 350 | 0.727 | Sbarufatti+ (2005) | bll | AMB | 0 | The source displays ambiguous characteristics of both BL Lac Objects and FRII radio galaxies (Landt+Bignall (2008)). The SDSS clearly shows forbidden [OII] and [OIII] lines, but Sbarufatti+ (2005) also reported the detection of MgII. The radio spectrum is flat above 1.4 GHz, but steep below this frequency. | ||
| J | PKS B | 0.852 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG2 J | 1.81 | Shaw+ (2009) | fsrq | FSRQ | 0 | SDSS | ||
| J | B3 | 0.365 | Cao+ (1999) | agn | MIS | 0 | SDSS. Classified as FRII by Kayanoki+Fukazawa (2022) | ||
| J | PKS B | 1.58 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bll | UNCL | 3 | - | ||
| J | OL 318 | 1.41 | Wills+Wills (1976) | fsrq | FSRQ | 0 | SDSS | ||
| J | GB6 J | 0.732 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OL 220 | 0.566 | Schmidt (1974) | fsrq | FSRQ | 0 | SDSS. Please note that ADS has scanned the first printing of the Schmidt’s paper, which do not include the table with the redshifts because of an error, but not the Errata Corrige, where the table is printed. It was necessary to retrieve the correct paper from our local library. | ||
| J | AT20G J | 0.589 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1H | 0.212 | Albert+ (2007) | bll | BLLAC | 0 | A value of appeared in Lin+ (1996): they referred to Hewitt+Burbidge (1993), but that paper referred to Wisniewski+ (1986), which in turn reported a featureless spectrum and no redshift. SDSS spectrum is inconclusive, but with a strange blue tail. | ||
| J | TXS | 0.678 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.70 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.683 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.689 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 7C | 0.379 | Galbiati+ (2005) | bcu | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.417 | SDSS | bcu | BLLAC | 0 | - | ||
| J | GB6 J | 1.54 | SDSS | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.584 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.794 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.95 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 B | 1.23 | Peterson+ (1978) | fsrq | FSRQ | 0 | Kraus+Gearhart (1975) reported , and this value remained in the literature for a while; it is not clear the reason of the mismatch. SDSS confirms Peterson’s redshift. | ||
| J | TXS | 0.664 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SDSS J | 0.660 | SDSS | bcu | AMB | 0 | The SDSS spectrum is galaxy-dominated, with strong [OII] and other weak lines. The LAT spectrum is quite soft (), suggesting a misaligned AGN, rather than a BLLAC, but the radio spectrum is flat, although there are no measurements below 1.4 GHz. | ||
| J | GB6 J | 0.452 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SDSS J | 0.566 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.771 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MS | 0.142 | Stocke+ (1991) | bll | AMB | 0 | SDSS. The optical spectrum is more FRI-like than BL Lac (Rector+ (1999)), while the remaining MW characteristics are of a BL Lac Object. | ||
| J | PMN J | - | - | bll | UNCL | 3 | - | ||
| J | RX J | 0.117 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013) | ||
| J | 4C | 1.25 | Hewitt+Burbidge (1993) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.671 | Muñoz+ (2003) | fsrq | FSRQ | 0 | The SDSS is noise-dominated, but it displays a clear emission line at Å corresponding to MgII. | ||
| J | RX J | 0.433 | SDSS | bll | BLLAC | 0 | - | ||
| J | RX J | 0.534 | Stadnik+Romani (2014) | bll | BLLAC | 1 | - | ||
| J | PKS | 1.57 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | 0.165 | SDSS | bll | SEY | 0 | - | ||
| J | NVSS J | 0.302 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.267 | Jones+ (2009) | bll | BLLAC | 0 | Although the 6dF measurement has , the Ca H+K and G band are clearly visible. Bauer+ (2000) reported an uncertain . | ||
| J | PKS | - | - | bll | BLLAC | 2 | Titov+ (2017) | ||
| J | GB6 J | 0.879 | Falco+ (1998) | bcu | FSRQ | 0 | - | ||
| J | GB6 J | 0.461 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.816 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 2MASS J | 0.875 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.715 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.240 | Falco+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 0.471 | Landt+ (2001) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.584 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.877 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | S5 | 0.123 | Stickel+Kühr (1993) | bll | FSRQ | 0 | - | ||
| J | 1ES | 0.361 | Polomski+ (1997) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.23 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.219 | Table A2 | bcu | UNCL | 1 | It seems to be the dominant galaxy in a cluster; Pierre+ (1994) and Bauer+ (2000) reported an uncertain of unknown origin. | ||
| J | B3 | 0.502 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 2MASS J | 0.681 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | S4 | 1.12 | Walsh+ (1979) | fsrq | FSRQ | 0 | SDSS | ||
| J | GB6 J | 0.211 | SDSS | bll | BLLAC | 0 | - | ||
| J | RX J | 0.448 | SDSS | bcu | BLLAC | 0 | Noisy spectrum, caveat. | ||
| J | S4 | 1.41 | SDSS | FSRQ | FSRQ | 0 | Stickel+Kuhr (1994) reported on the basis of one individual emission line identified as MgII. | ||
| J | PMN J | 1.13 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.883 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | 2MASS J | - | - | bcu | UNCL | 3 | - | ||
| J | OL 256 | 0.595 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.529 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.82 | Jauncey+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.302 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.312 | Stickel+Kühr (1989) | fsrq | CLAGN | 0 | Jauncey+ (1979) reported a featureless continuum with , while the Stickel & Kühr’s (1989) spectrum showed lines with . | ||
| J | GB6 J | 1.14 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | PKS B | 1.07 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 1.01 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.490 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.512 | Ching+ (2017) | bcu | BLLAC | 0 | - | ||
| J | PKS B | 0.525 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.666 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.740 | Paiano+ (2021) | bll | BLLAC | 0 | SDSS reported on the basis of an extremely weak feature identified as MgII. | ||
| J | 1RXS J | 1.156 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.347 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.208 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 0.390 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.3 | Table A2 | bll | UNCL | 1 | - | ||
| J | RBS 895 | 0.660 | Ching+ (2017) | bcu | BLLAC | 0 | Boyle+ (1990) suggested an uncertain on the basis of a single feature identified as Mg II and low S/N spectrum. | ||
| J | B2 A | 0.559 | White+ (2000) | fsrq | CLAGN | 0 | Hook+ (1996) reported a featureless spectrum with an upper limit to the lines Å. White+ (2000) measured the redshift by using lines with Å. SDSS displays a prominent MgII line. | ||
| J | NVSS J | 1.21 | Table A2 | bll | BLLAC | 1 | Paiano+ (2021) | ||
| J | S5 | 1.26 | Eckart+ (1986) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.841 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS B | 2.13 | Baker+ (1999) | fsrq | FSRQ | 0 | - | ||
| J | 7C | 0.249 | Caccianiga+ (2002) | bcu | AMB | 0 | SDSS. Caccianiga+ (2002) classified it as Type 2, which are objects with only narrow emission lines (Seyfert 2, Narrow-Emission Line Radio Galaxies, LINERS, starburst), but Caccianiga+ (2004) reported a core dominance parameter . The steep gamma-ray spectrum () favors a radio galaxy. | ||
| J | NVSS J | 0.254 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | GB6 J | 0.437 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 0.643 | Zhou+ (2004) | bcu | AMB | 0 | Zhou+ (2004) also proposed that the source could be a binary black hole on the basis of double-peaked lines, but Jaiswal+ (2019) suggested that the line profiles are due to the interaction of the jet with the NLR. SDSS: please note an error in the redshift evaluation from the automatic pipeline, where the H+[OIII] complex is incorrectly identified as H+[NII] complex, with a clear mismatch of the frequencies of many other lines. | ||
| J | GALEXASC J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.595 | Murdoch+ (1984) | fsrq | NLS1 | 0 | FWHM(H) km/s, [OIII]/H. | ||
| J | S5 | 1.15 | Stickel+ (1996) | FSRQ | FSRQ | 0 | - | ||
| J | GB6 J | 0.327 | Paggi+ (2014) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.402 | SDSS | bll | BLLAC | 0 | - | ||
| J | MG1 J | 0.949 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 1.22 | Clowes+Campusano (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | RBS 909 | 0.498 | Beckmann+ (2003) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 1.43 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | OL 282 | 1.30 | Wills+Wills (1976) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.265 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS | ||
| J | 2MASX J | 0.223 | SDSS | bcu | BLLAC | 0 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Marchesini+ (2019) | ||
| J | GB6 J | 0.140 | Gioia+ (1990) | bll | MIS | 0 | SDSS. Capetti+ (2017) display an image of radio structure showing a clear bipolar large scale jet (>30 kpc). | ||
| J | WN B | 0.224 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 2.64 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 87GB | 0.316 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | RX J | 0.755 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | RX J | 0.236 | Appenzeller+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | S5 | 2.49 | Xu+ (1994) | fsrq | FSRQ | 0 | - | ||
| J | SDSS J | 0.761 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS B | 1.13 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.092 | Bade+ (1994) | bll | BLLAC | 0 | - | ||
| J | B3 | 1.31 | SDSS | bll | BLLAC | 0 | - | ||
| J | 4C | 0.892 | Kraus+Gearhart (1975) | BLL | FSRQ | 0 | SDSS | ||
| J | S5 | 0.706 | Xu+ (1994) | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.254 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.143 | Bade+ (1998) | BLL | BLLAC | 0 | SDSS. Marcha+ (1996) reported by identifying as [OIII] complex two strong lines at Å(observation done in 1992). These lines were never confirmed. Laurent-Muehleisen+ (1998) observed the source in 1994-1995 and found a featureless spectrum. Bade’s observation was done in 1997, but no lines around Å(the same in SDSS spectrum). | ||
| J | PKS | 0.581 | Sbarufatti+ (2009) | bll | BLLAC | 0 | - | ||
| J | PKS B | 0.611 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | MG2 J | 0.393 | Hook+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.225 | Beckmann+ (2003) | bll | BLLAC | 0 | - | ||
| J | RX J | 1.15 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | CRATES J | 0.941 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CLASS J | 0.577 | Table A2 | fsrq | UNCL | 1 | - | ||
| J | GB6 J | 0.690 | SDSS | fsrq | NLS1 | 0 | FWHM(H) km/s, Rakshit+ (2017). | ||
| J | RX J | 0.545 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 B | 0.384 | Everett+Wagner (1995) | fsrq | FSRQ | 0 | SDSS. Maithil+ (2020) suspect it might be a CSS. | ||
| J | TXS | 0.913 | Afanas’ev+ (2003) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1ES | 0.186 | Remillard+ (1989) | bll | BLLAC | 0 | Kirhakos+Steiner (1990) proposed and associated it to NGC 3513, which in turn is distant! It seems clearly to be an error. Remillard’s redshift was later confirmed by Falomo+ (1993) and many others studies. | ||
| J | NVSS J | 0.275 | Colless+ (2001) | bll | BLLAC | 0 | SDSS shows a nearby object, but without spectrum. Might be an interacting system. To be checked. | ||
| J | SDSS J | 0.771 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | MG1 J | 0.295 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | Mkn 421 | 0.0308 | Ulrich+ (1975) | BLL | BLLAC | 0 | - | ||
| J | 7C | - | - | bcu | UNCL | 3 | - | ||
| J | GB6 J | 0.099 | SDSS | bll | BLLAC | 0 | In the compact group of galaxies Shakhbazian 7 (Shakhbazian 1973). | ||
| J | MG2 J | 0.842 | Glickman+ (2007) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.242 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.412 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2017) | ||
| J | PKS | 1.60 | Peterson+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.610 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | PKS | 0.740 | Caccianiga+ (2000) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.386 | Table A2 | bll | BLLAC | 1 | SDSS. Bauer+ (2000) reported with the flag “uncertain”, and never confirmed. | ||
| J | NVSS J | 0.693 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1ES | 0.46 | Sbarufatti+ (2005) | bll | BLLAC | 1 | Sbarufatti+ (2009) reported in an ATel, a spectroscopic based on the detection of the Ca H&K break, but the value was not confirmed in a subsequent paper (Landoni+ (2013)). Paiano+ (2017) still found a featureless spectrum. | ||
| J | NVSS J | 0.398 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.513 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.579 | Table A2 | bll | BLLAC | 1 | Laurent-Muehleisen+ (1998) | ||
| J | CRATES J | 0.860 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | FBQS J | 0.549 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | WISE J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.212 | Bade+ (1998) | bll | BLLAC | 0 | - | ||
| J | SDSS J | 0.577 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.421 | SDSS | bll | BLLAC | 0 | - | ||
| J | TXS | 1.95 | Hewitt+Burbidge (1993) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.779 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 2.08 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.04 | Croom+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.437 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.049 | Burbidge+Strittmatter (1972) | rdg | MIS | 0 | SDSS. Dumbbell, FRI, Liuzzo+ (2009), Liuzzo+ (2010). | ||
| J | RBS 958 | 0.138 | Schwope+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | RX J | 0.451 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.836 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.360 | White+ (2000) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.677 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.935 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.715 | Table A2 | agn | UNCL | 1 | - | ||
| J | PKS | 0.713 | Tritton (1971) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.74 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | OM 127 | 2.12 | Schmidt (1966) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.412 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.335 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 970 | 0.053 | Table A2 | bll | BLLAC | 1 | Perlman+ (1996) reported an uncertain on the basis of Ca H&K break, but this value was challenged by Falomo+Kotilainen (1999), on the basis of the imaging of the host galaxy (not resolved). No further observation confirmed Perlman’s value. The latest observation by Paiano+ (2017) still found a featureless spectrum. | ||
| J | MGC 0019706 | 0.0993 | Liske+ (2003) | bcu | MIS | 0 | Sadler+ (2014) classified it as FRI Wide-Angle-Tail radio galaxy. | ||
| J | PKS | 1.30 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.200 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | NVSS J | 0.146 | Jones+ (2009) | fsrq | FSRQ | 0 | 6dF | ||
| J | WN B | 1.33 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.690 | Table A2 | bll | BLLAC | 1 | Massaro+(2015) | ||
| J | SDSS J | 0.523 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | OM 235 | 1.55 | Shaw+ (2012) | fsrq | CLAGN | 0 | SDSS confirms Shaw’s value. Sowards-Emmerd+ (2005) and Healey+ (2008) reported a featureless spectrum. Mahabal+ (2009) reported on a likely wrong identification of Ly and CIV lines. | ||
| J | CRATES J | 0.795 | SDSS | bcu | BLLAC | 0 | There is a mismatch () between the CRATES coordinates and the columns RA_counterpart and DEC_counterpart in the 4FGL. The former have no entries both in SIMBAD and NED, while the latter are coincident with SDSS J. Hook+ (1996) reported a featureless spectrum. | ||
| J | AT20G J | 0.638 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 1.00 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.520 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.461 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 0.284 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | 4C | 0.133 | Sargent (1973) | fsrq | AMB | 0 | SDSS with strong narrow forbidden lines and weak H. Marchã+ (1996) suggested a candidate BL Lac; Zirbel+Baum (1995) suggested a FRII radiogalaxy. The radio spectrum is flat, but the gamma-ray spectrum is on the borderline between a BL Lac and a FSRQ. | ||
| J | 1RXS J | 0.279 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.572 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.05 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 2.89 | Walsh+ (1984) | fsrq | FSRQ | 0 | SDSS | ||
| J | MRC | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.884 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 1.80 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.963 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | CRATES J | 0.633 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.920 | Peña-Herazo+ (2017) | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.817 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.586 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 1.19 | Burbidge+Kinman (1966) | fsrq | FSRQ | 0 | 6dF | ||
| J | LEDA 566417 | 0.150 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | NVSS J | 0.151 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.167 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | B2 | 1.74 | Xu+ (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.623 | Table A2 | bcu | UNCL | 1 | Grazian+ (2002) classified it as a star (but no spectrum published). Radio: there is only the NVSS detection ( mJy at 1.4 GHz) | ||
| J | 1RXS J | 0.360 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.266 | Drinkwater+ (1997) | bcu | MIS | 0 | Classified as radiogalaxy by Angioni+ (2019) and Homan+ (2021). | ||
| J | SUMSS J | 0.210 | Peña-Herazo+ (2017) | bcu | BLLAC | 0 | - | ||
| J | PKS B | 0.678 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.0587 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.571 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | CRATES J | 0.757 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.273 | Sadler+ (2002) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | 1.34 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.286 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.134 | Bade+ (1994) | bll | BLLAC | 0 | SDSS | ||
| J | Mkn 180 | 0.0458 | Ulrich (1978) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.154 | White+ (2000) | bll | SEY | 0 | SDSS | ||
| J | PKS | 0.486 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.600 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.315 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 1.30 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | CRATES J | 2.36 | SDSS | bcu | FSRQ | 0 | - | ||
| J | RX J | 0.628 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.244 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | 1RXS J | 0.598 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.360 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | MG1 J | 0.734 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | GB6 J | 0.322 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 3C 264 | 0.022 | Schmidt (1965) | rdg | MIS | 0 | SDSS, classified as FRI by Balmaverde+ (2021) | ||
| J | B3 A | 0.300 | Hook+ (1996) | fsrq | SEY | 0 | SDSS, optical spectrum with strong narrow lines, flat radio spectrum. | ||
| J | RBS 1029 | 0.168 | Machalski+Condon (1999) | bll | BLLAC | 0 | SDSS | ||
| J | 87GB | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.34 | White+ (1988) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.294 | Mahony+ (2011) | bcu | FSRQ | - | - | ||
| J | PKS | 1.06 | Table A2 | fsrq | BLLAC | 1 | Wilkes+ (1983) reported flagged as uncertain. It was never confirmed; nonetheless, it propagated into the literature as certain value. | ||
| J | S4 | 1.09 | Vigotti+ (1990) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 1.05 | Stickel+ (1989) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.963 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.34 | Wilkes+ (1983) | fsrq | FSRQ | 0 | Binary? Djorgovski+ (1987) | ||
| J | TXS | 0.866 | Bade+ (1995) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.654 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NGC 3894 | 0.0108 | Kelton (1980) | rdg | MIS | 0 | LAMOST. E/S0 host galaxy, twin jets, CSO? Taylor+ (1998) | ||
| J | 7C | 1.24 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.478 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RX J | 0.402 | Beckmann+ (2003) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | OM 280 | 0.209 | Truebenbach+Darling (2017) | bll | BLLAC | 0 | Please note a misleading comment in the Vizier catalog, where the redshift is indicated as lower limit from the OCARS catalog, while in the individual note in the article is written that the value is measured from emission lines detected in the spectrum observed by the authors. | ||
| J | RBS 1040 | 0.519 | Table A2 | bll | BLLAC | 1 | There is one measurement by White+ (2000): based on a single weak line identified as MgII. This line was never confirmed by newer observations (Shaw+ 2013; Paiano+ 2020). The positions are consistent each others, and also the optical magnitudes, indicating that the source was observed at the same flux level. Curiously, the SDSS spectrum shows a feature flagged as an artifact more or less at the same wavelenght. Both White’s spectrum and the SDSS one were taken at the Apache Point Observatory (11 years difference): perhaps it is a local artifact. | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.609 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | TXS | 0.702 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.636 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.700 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.441 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS B | 2.37 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | B2 A | 1.39 | White+ (2000) | fsrq | FSRQ | 0 | SDSS. | ||
| J | S5 | 1.25 | Kühr+ (1981) | fsrq | FSRQ | 0 | - | ||
| J | PKS B | 0.269 | Osmer+Hewett (1991) | bcu | FSRQ | 0 | - | ||
| J | 4C | 0.334 | Lynds+Wills (1968) | FSRQ | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.683 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.410 | SDSS | bll | SEY | 0 | - | ||
| J | B3 | 0.923 | Hook+ (1996) | fsrq | NLS1 | 0 | Henstock+ (1997) measured FWHM(H) km/s. They had a spectrum with better S/N than SDSS at Å. | ||
| J | RX J | 1.12 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.254 | Bauer+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.437 | Table A2 | bll | UNCL | 1 | SIMBAD gives from Mahony+ (2010), which in turn refer to a paper in preparation. However, nothing published was found in the following years. | ||
| J | NVSS J | 0.328 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | SDSS J | 0.992 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 1.15 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.890 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB1 | 2.04 | Henstock+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | - | - | bcu | AMB | 2 | The ambiguity derives from two nearby () optical counterparts: SDSS-1 at and SDSS-2 at . There is only one radio counterpart from FIRST ( mJy), which could be of one of the two galaxies or both (resolution ). | ||
| J | GB6 J | 0.873 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.565 | Wright+ (1979) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.617 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | Ton 599 | 0.725 | Burbidge (1968) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.368 | Table A2 | bll | UNCL | 1 | - | ||
| J | 87GB 115739.6+021927 | 0.635 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.656 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.430 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.698 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.755 | Glickman+ (2007) | bcu | AMB | 0 | No spectrum available, but Glickman+ (2012) classified it as Narrow-Line AGN or Starburst, with [OIII]/H. However, radio spectrum is flat . NLS1? | ||
| J | OM 198 | 0.601 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B3 | 0.297 | SDSS | bll | BLLAC | 0 | Please note it is only far from NGC 4051 | ||
| J | NVSS J | 0.771 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.381 | Wright+ (1979) | fsrq | NLS1 | 0 | FWHM(H) km/s, confirmed by Wilkes (1986), who found FWHM(H) km/s. Optical spectrum available here from Monroe+ (2016) | ||
| J | TXS | 0.0631 | Ulrich (1976) | bcu | MIS | 0 | Radiogalaxy in the cluster A1452. Galaxy dominated optical spectrum. Steep radio spectrum, complex radio morphology: wide-angle tail? head-tail? (Miley+Harris 1977, Sakelliou+Merrifield 2000). | ||
| J | SBS | 0.065 | Martel+Osterbrock (1994) | bll | SEY | 0 | SDSS, LINER, S0 host galaxy. | ||
| J | TXS | 1.2 | Flesch (2021) | bcu | FSRQ | 1 | Flesch also classified the source as quasar. | ||
| J | PMN J | 0.227 | Peña-Herazo+ (2017) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.296 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS | ||
| J | 1RXS J | 0.184 | Mamon+ (2001) | bll | BLLAC | 0 | Landt+ (2001) set the same value as tentative, but later (Landt+Bignall 2008) confirmed it. | ||
| J | MG1 J | 1.95 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.790 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | SDSS J | 1.01 | SDSS | bcu | FSRQ | 0 | SDSS shows a possible contaminating source at South. There is a LAMOST spectrum almost featureless, perhaps a BL Lac (radio emission not resolved, confusion with the above cited source). However, the soft gamma-ray spectrum () suggests that the responsible of the gamma-ray emission is the quasar. | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | AT20G J | 1.01 | Wilkes+ (1983) | fsrq | FSRQ | 0 | LAMOST | ||
| J | NVSS J | 0.760 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | GB6 J | 0.618 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | RGB J | 0.275 | SDSS | bll | MIS | 0 | Ultrasteep radio spectrum (, Bornacini+ 2010), classified as FRII by Miraghei+Best (2017) | ||
| J | TXS | 1.34 | Shaw+ (2012) | fsrq | NLS1 | 0 | SDSS, classified as NLS1 by Rakshit+ (2021). It is the farthest NLS1. | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | B3 | 0.505 | Table A2 | bll | BLLAC | 1 | Shaw+ 2013 | ||
| J | 2MASS J | 0.486 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 1.44 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | MG1 J | 0.845 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | FIRST J | 0.616 | Rector+ (1999) | bll | BLLAC | 0 | Stocke+ (1991) reported on the basis of a strong line identified as [OII], but a reanalysis of the same spectrum by Rector+ (1999) resulted in in the basis of the Ca H+K break. Landt+ (2002) reported , but it seems a typo, because they refer to Rector+ (2000), which in turn refer again to Rector+ (1999). | ||
| J | NVSS J | 0.760 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.453 | Beckmann+ (2003) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 0.666 | Desai+ (2019) | bcu | BLLAC | 0 | - | ||
| J | 1RXS J | 0.244 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.555 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RBS 1080 | 0.278 | Fischer+ (1998) | bll | BLLAC | 0 | - | ||
| J | 4C | 1.14 | Lynds+Wills (1972) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.734 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | - | - | bll | UNCL | 3 | - | ||
| J | PKS B | 0.149 | Murdoch+ (1984) | bcu | NLS1 | 0 | FWHM(H) km/s. | ||
| J | TXS | 1.13 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | 0.136 | Perlman+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | 7C | 0.504 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | IVS B | 0.622 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | - | - | bcu | UNCL | 3 | Source hidden by an extremely bright star in foreground | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | TXS | 0.094 | Bauer+ (2000) | bll | SEY | 0 | SDSS | ||
| J | 1RXS J | 0.219 | Table A2 | bll | BLLAC | 1 | Huchra+ (1992) reported and a BLLAC classification (see also CfA ZCat), but Bauer+ (2000) wrote an uncertain . LAMOST inconclusive | ||
| J | B2 | 0.129 | Paiano+ (2017) | BLL | BLLAC | 0 | Padovani+ (1995) reported from Murphy+ (1993), which in turn wrote that they took it from NED; Bade+ (1998) reported from a paper in preparation by Perlman, but no such published paper was found. The Paiano’s spectrum seems to be the first ever published. | ||
| J | PKS | 0.419 | Dunlop+ (1989 | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.498 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013). Downes+ (1986) reported from a private communication of Ann Savage, but neither published spectrum nor confirmation of this value were found. | ||
| J | ON 428 | 1.07 | Stickel+Kuhr (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.150 | Klindt+ (2017) | bll | BLLAC | 0 | - | ||
| J | NGC 4261 | 0.00734 | Huchra+ (1983) | rdg | MIS | 0 | FRI, Chiaberge+ (1999) | ||
| J | NVSS J | 0.138 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.299 | SDSS | bll | BLLAC | 0 | - | ||
| J | 87GB | 0.851 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB2 J | 0.643 | Hewett+Wild (2010) | bll | BLLAC | 1 | - | ||
| J | S5 | 0.451 | Stickel+Kuhr (1996) | fsrq | AMB | 0 | No classification is possible, because neither a spectrum, nor line information were published. | ||
| J | 2MASS J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PG | 0.184 | Bade+ (1998) | bll | BLLAC | 0 | Bade reported a personal communication by Perlman, who did not publish the spectrum, but SDSS confirmed the value. Before Bade, a value of was often adopted, and it was estimated on the basis of the imaging of the host galaxy (Weistrop+ 1981). | ||
| J | W Comae | 0.102 | Weistrop+ (1985) | bll | BLLAC | 0 | The value was challenged by Finke+ (2008), because they did not detect any feature. However, Paiano+ (2017) confirmed the Weistrop’s value. Additionally, SDSS spectrum clearly shows [OIII] line at Å, but the automatic pipeline curiously missed it. The manual analysis by Shaw+ (2013) revealed it. It is likely that the featureless spectrum taken by Finke was due to high jet activity. | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | 4C | 0.966 | Wilkes+ (1983) | fsrq | FSRQ | 0 | SDSS | ||
| J | SDSS J | 1.15 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | MG1 J | 0.998 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.200 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | RX J | 0.261 | SDSS | bll | BLLAC | 0 | - | ||
| J | S5 | 0.469 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013). Some papers reported from the OCARS catalog, which in turn refers to NED and SIMBAD. Origin of this value is unknown. | ||
| J | SBS | 1.06 | Stepanian (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.375 | Paiano+ (2017) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.479 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MS | 0.219 | Stocke+ (1991) | bll | BLLAC | 0 | SDSS | ||
| J | PKS 1221-82 | - | - | bcu | UNCL | 3 | - | ||
| J | 4C | 0.434 | Burbidge+Kinman (1966) | FSRQ | FSRQ | 0 | SDSS. It might be a CLAGN (changing SED), see Foschini+ (2011) | ||
| J | B3 | 0.958 | SDSS | bll | AMB | 0 | The SDSS spectrum (taken on MJD 57785) is rather noisy, but the MgII line seems to be reliable. Previous SDSS spectra were too much noisy and Shaw+ (2013) reported only lower limits (MJD 53112). Sowards-Emmerd+ (2003) took another spectrum and reported , with a FSRQ identification. They identified the feature at Å as CIII, while SDSS identified it as MgII. The latter seems to be more reliable, although all the available spectra are rather noisy; therefore, we decided for the AMB classification. | ||
| J | 4C | 0.956 | Hewitt+Burbidge (1987) | fsrq | FSRQ | 0 | Hewitt+Burbidge (1987) referred to Bolton+Wall (1970), but the latter did not report any redshift. However, the value is confirmed by SDSS | ||
| J | 1RXS J | 0.260 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | 1RXS J | 0.272 | Table A2 | bcu | UNCL | 1 | - | ||
| J | AT20G J | 1.72 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.294 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.163 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2021). Chang+ (2019) reported as a firm spectroscopic measurement, but it seems to be derived from SDSS-DR13, which is not firm, as there are other values in the other releases (SDSS). | ||
| J | PMN J | 0.456 | Mao (2011) | bll | BLLAC | 1 | - | ||
| J | PKS | 0.110 | Massardi+ (2008) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.72 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | 3C 273 | 0.158 | Schmidt (1963) | FSRQ | FSRQ | 0 | LAMOST (1, 2, 3) | ||
| J | ON 246 | 0.555 | Table A2 | bll | BLLAC | 1 | Nass+ (1996) reported (neither spectrum nor line information published), but Laurent-Muehleisen+ (1999) wrote that it is incorrect on the basis of a personal communication by Bade (1998). Beckmann+ (2003), including Bade, confirmed (again without spectrum and/or line information). More recent observations by Shaw+ (2013), Massaro+ (2015), and Paiano+ (2017) all failed to confirm the redshift and all reported featureless spectra. Perhaps the jet activity overwhelmed the line emission during the recent observations, but it is not possible to establish the reliability of old observations, since no spectra were published. | ||
| J | M 87 | 0.00436 | Humason+ (1956) | rdg | MIS | 0 | See McConnell+Ma (2013) for more recent results on z | ||
| J | WISEA J | SDSS | bll | MIS | 0 | Classified as FRII by Kozieł-Wierzbowska+Stasińska (2011). | |||
| J | GB6 J | 0.256 | Wolter+ (1997) | bll | BLLAC | 0 | SDSS | ||
| J | MS | 0.163 | Stocke+ (1991) | bll | BLLAC | 0 | SDSS | ||
| J | B2 | 0.236 | Beckmann+ (2003) | bll | BLLAC | 0 | White+ (2000) first reported on the basis of a large (doubtful) feature centered at Å identified as MgII. Landt+Bignall (2008) found a featureless spectrum and set . Shaw+ (2013) confirmed the Beckmann’s value, but with an uncertainty flag. SDSS inconclusive (but it does not show the large feature reported by White) | ||
| J | GB1 | 1.59 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.719 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.207 | Falco+ (1998) | bll | AMB | 0 | SDSS. Steep radio spectrum from Specfind, likely a MIS, but Caccianiga+ (2002) classified it as type 0 (BL Lac), passive elliptical galaxy. | ||
| J | NVSS J | 0.581 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | NVSS J | 0.629 | Table A2 | bcu | UNCL | 1 | Paiano+ (2019) suggested a different counterpart on the basis of the Swift/XRT follow-up, which is distant from the 4FGL counterpart. Paiano’s source is classified as Seyfert 2 galaxy at , but no radio detection is reported. | ||
| J | RX J | 0.389 | SDSS | bll | BLLAC | 0 | Hook+ (1998) reported a featureless spectrum, likely due to the jet activity. | ||
| J | RX J | 0.700 | Bade+ (1998) | bll | BLLAC | 0 | - | ||
| J | 1H | 0.297 | Gioia+ (1984) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 0.361 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2020) | ||
| J | PMN J | 0.703 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | TXS | 0.293 | Jones+ (2009) | fsrq | FSRQ | 0 | Hewitt+Burbidge (1993) reported on the basis of a personal communication by Wills+ (1987), who identified two features as CIII and CIV (spectrum never published). However, the 6dF spectrum clearly shows prominent emission lines of the H-[OIII] complex. [OIII] is clearly stronger than H, which in turn displays a red wing. | ||
| J | PKS | 0.552 | Table A2 | bll | BLLAC | 1 | SDSS. White+ (1998) suggested a tentative on the basis of a few weak lines (MgII, [OIII], H) measured on a noisy spectrum (not published). This value has been always taken for granted, although never confirmed. | ||
| J | MG1 J | 1.76 | Halpern+ (2003) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 1.18 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.619 | SDSS | bcu | BLLAC | 0 | Borderline radio spectrum. | ||
| J | RX J | 0.266 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RX J | 0.133 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013) | ||
| J | 1ES | 1.56 | Table A2 | bll | BLLAC | 1 | Perlman+ (1996) reported in the basis of the host galaxy features (spectrum unpublished), but it was never confirmed. Sbarufatti+ (2006) and Landoni+ (2013) both reported featureless spectra. SDSS inconclusive. | ||
| J | 1RXS J | 0.485 | Table A2 | bll | UNCL | 1 | - | ||
| J | S5 | 0.074 | Marchã+ (1996) | bcu | BLLAC | 0 | - | ||
| J | SDSS J | 1.06 | Table A2 | bcu | AMB | 1 | SDSS spectrum is quite noisy, but it shows an emission line at Å, which is unlikely identified as Ly. If it is MgII, the tentative redshift would be ; the source would be a FSRQ. | ||
| J | Ton 116 | 0.5 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | PMN J | 0.788 | Table A2 | bcu | BLLAC | 1 | Healey+ (2008) | ||
| J | SUMSS J | 0.301 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.456 | SDSS | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.542 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.710 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.386 | Vanden Berk+ (2002) | bll | BLLAC | 0 | See also Gal-Yam+ (2002). SDSS | ||
| J | PKS | 0.638 | Wilkes (1986) | fsrq | NLS1 | 0 | Wilkes reports also FWHM(H) km/s and FWHM(H) km/s. | ||
| J | RX J | 0.569 | Landoni+ (2018) | bll | BLLAC | 0 | SDSS automatic pipeline fails to catch the narrow emission line at Å, identified as [OIII] by Landoni. | ||
| J | PG | 0.508 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | RX J | 0.351 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | SDSS | ||
| J | 87GB | 1.86 | SDSS | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.103 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GALEXASC J | 0.223 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.883 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.955 | Sandrinelli+ (2013) | bll | BLLAC | 0 | SDSS noisy, but confirms the z. | ||
| J | NVSS J | 0.304 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.245 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS (quite noisy) | ||
| J | TXS | 0.414 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.606 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 0.59 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | 1RXS J | 0.179 | Piranomonte+ (2007) | bll | BLLAC | 0 | 6dF | ||
| J | MG1 J | 0.066 | Grogin+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | 1RXS J | 0.515 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.7 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.525 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | ON 187 | 0.872 | Bolton+ (1965) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.0411 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | 3C 279 | 0.536 | Marziani+ (1996) | FSRQ | FSRQ | 0 | First redshift by Burbidge+Rosenberg (1965) | ||
| J | PMN J | 0.0579 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | RX J | 0.531 | Shaw+ (2013) | bll | BLLAC | 0 | There is a tentative reported by Braccesi+ (1970) on the basis of an unpublished work by Lynds+ (1969). This value was taken for granted and reported in many catalogs, until the Shaw’s measurement. | ||
| J | 1ES | 0.141 | Perlman+ (1996) | bll | BLLAC | 0 | SDSS. Please note that there is a typo in Table 1 of Perlman+ (1996), where is , but his Table 4 reported the correct value of , also consistent with the spectrum published in his Figure 4. | ||
| J | ON 393 | 0.806 | SDSS | fsrq | FSRQ | 0 | Healey+ (2008) reported on the basis of their own spectroscopy (no spectrum published). It is likely that they have misidentified the most prominent line ( Å) as CIII] instead of MgII. | ||
| J | NVSS J | 0.204 | Table A2 | bll | BLLAC | 1 | SDSS spectrum is extremely noisy and calculated , based on features identified as Ca H+K and H+[NII]. [OIII] is corresponding to a strong absorption feature. No other published spectra. | ||
| J | PKS B | 1.96 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.441 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 1194 | 0.418 | Paiano+ (2021) | bll | BLLAC | 0 | Scwhope+ (2000) proposed a BLLAC classification with flagged as uncertain. No spectrum published. | ||
| J | PKS | 1.31 | Dekker+D’Odorico (1984) | fsrq | FSRQ | 0 | Note: the full text file available on NASA/ADS is not complete. | ||
| J | PKS B | 0.481 | Sbarufatti+ (2005) | bll | FSRQ | 0 | Drinkwater+ (1997) took a broad-band spectrum ( Å) and reported on the basis of two strong emission lines at and Å, but they did not write the identification of the lines (the latter might be H). By taking for good the Sbarufatti’s value, the lines in the Drinkwater spectrum should be HeI and H, respectively. The lack of these two lines in Sbarufatti’s spectrum is due to a smaller waveband (∼4000–8000 Å). | ||
| J | NVSS J | 0.237 | Table A2 | bcu | UNCL | 1 | - | ||
| J | LEDA 4075145 | - | - | bll | BLLAC | 2 | 6dF | ||
| J | NVSS J | 0.223 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | SDSS J | 0.834 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | OW 197 | 1.11 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | GB6 J | 0.520 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MG2 J | 1.01 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.572 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.568 | Hook+ (1996) | bcu | AMB | 0 | It is not possible to classify this source, because there is neither spectrum published, nor indication of the line strengths. The spectrum is missing in the Hook’s paper: misprint? Additionally, Falco+ (1998) did not publish the spectrum and reported a list of lines, but without any indication of equivalent width. They also wrote that the host is a late-type galaxy, which suggests a possible SEY/NLS1 classification. | ||
| J | TXS | 0.141 | SDSS | bll | MIS | 0 | FRI, Capetti+ (2017). Warning: the 4FGL coordinates differ by from the radio position of the counterpart. | ||
| J | TXS | 1.09 | Healey+ (2008) | bll | CLAGN | 0 | Healey measured the redshift and classified the source as FSRQ, but neither spectrum, nor line information are published. Hentstock+ (1997) found a featureless spectrum, and so is the SDSS. | ||
| J | MG2 J | 0.993 | Glickman+ (2007) | bll | BLLAC | 0 | Shaw+ (2013) confirmed BLLAC classification, but on the basis of a featureless spectrum, likely due to an increased jet activity. | ||
| J | PMN J | 1.66 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | WISE J | 0.940 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.26 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Shaw+ (2013), Masetti+ (2013) | ||
| J | PKS | 1.25 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | - | ||
| J | PKS B | 0.938 | Table A2 | bcu | UNCL | 1 | - | ||
| J | IERS B | 0.785 | SDSS | nlsy1 | NLS1 | 0 | Classified as NLS1 by Zhou+ (2006) | ||
| J | S5 | 0.610 | Table A2 | bll | UNCL | 1 | - | ||
| J | 2MASS J | 0.376 | SDSS | bll | MIS | 0 | Steep radio spectrum, classified as one-sided radio galaxy by Sikora+ (2013) | ||
| J | TXS | 0.086 | Afanasiev+ (2003) | rdg | MIS | 0 | SDSS. Classified as FRI by Miraghei+Best (2017) and Capetti+ (2017) | ||
| J | PKS | 0.126 | Grandi (1983) | rdg | MIS | 0 | Grandi suggested a classification as BLRG, but the H is rather weak and [OIII] lines are strong (obscuration?). Eracleous+Halpern (1994, 2004) correctly identified it as NLRG | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Titov+ (2017) | ||
| J | 5C | 1.05 | Vermeulen+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | B3 | 0.694 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS | ||
| J | 4C | 0.659 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013) | ||
| J | TXS | 0.140 | Bauer+ (2000) | bll | BLLAC | 0 | - | ||
| J | OP 313 | 0.996 | Perry+ (1978) | fsrq | FSRQ | 0 | SDSS | ||
| J | CRATES J | 0.226 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.926 | Henstock+ (1997) | fsrq | NLS1 | 0 | SDSS. Henstock reported FWHM(H) ∼ 22/9371 Å ∼700 km/s, but both their spectrum and SDSS one have H in the extreme red and noisy part of the spectrum. The complex H+[OIII] is quite contaminated. | ||
| J | RX J | 0.384 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | RX J | 1.64 | Machalski+Engels (1994) | fsrq | FSRQ | 0 | SDSS. Puchnarewicz+ (1997) set on the basis of a weak feature (only upper limits on EW and luminosity were available; no spectrum published) identified as CIII]. That work was in the framework of the ROSAT International X-ray/Optical Survey (RIXOS, FID 265, Source 1). However, later, in the definitive catalogue, Mason+ (2000) adopted Machalski+Engels’ value. | ||
| J | MG2 J | 0.724 | Table A2 | bcu | MIS | 1 | Classified as FRII by van Velzen+ (2015) on the basis of radio morphology. Steep radio spectrum. | ||
| J | FIRST J | 0.550 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.375 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) suggested a tentative based on a single weak feature identified as MgII (spectrum published). It is flagged as uncertain. | ||
| J | GB | 0.638 | Sokolovsky+ (2014) | bcu | AMB | 0 | Falco+ (1998) proposed an uncertain , while Healey+ (2008) reported and a FSRQ classification. Sokolovsky+ (2014) found that the AGN has and is behind a foreground galaxy at . The spectrum is rather ambiguous and does not allow a reliable classification. | ||
| J | NVSS J | 0.391 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 0.824 | Sowards-Emmerd+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 1.26 | Table A2 | bll | BLLAC | 1 | Landoni+ (2020) | ||
| J | TXS | 0.484 | Table A2 | bll | BLLAC | 1 | Paggi+ (2014) | ||
| J | MS | 0.108 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | 6C B | 0.573 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.406 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.200 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | PKS | 1.21 | Jauncey+ (1982) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.586 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | TXS | 0.920 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum, might it be a MIS? | ||
| J | S4 | 1.05 | Schmidt (1977) | fsrq | FSRQ | 0 | SDSS | ||
| J | 6C B | 0.895 | Table A2 | bcu | UNCL | 1 | - | ||
| J | AT20G J | 0.622 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.976 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.18 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.573 | Schwope+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PKS B | 0.891 | Bolton+ (1968) | bcu | MIS | 0 | SDSS. Steep radio spectrum. Classified as CSS by Dallacasa+ (1998) | ||
| J | NVSS J | 0.155 | Table A2 | bll | UNCL | 1 | - | ||
| J | TXS | 0.946 | Sowards-Emmerd+ (2003) | fsrq | FSRQ | 0 | SDSS. Shaw+ (2012) reported FWHM(H) km/s, while Rakshit+ (2020) found FWHM(H) km/s, and Wu+Shen (2022) measured FWHM(H) km/s. The profile of H and MgII is clearly distorted, with an apparent red wing, therefore the NLS1 classification should not apply. It seems to be a case similar to 4FGL J = PKS . | ||
| J | PKS | 2.03 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.396 | SDSS | bll | BLLAC | 0 | - | ||
| J | S5 | 0.934 | Table A2 | fsrq | UNCL | 1 | Brizten+ (2007) reported a tentative from a private communication by R. Vermeulen. However, no spectrum was ever published in the following years. This value has been taken for granted by other subsequent papers. | ||
| J | NVSS J | 0.326 | SDSS | fsrq | CLAGN | 0 | Álvarez Crespo+ (2016) reported a featureless spectrum (observation done on 2014/02/05, while SDSS done on 2012/02/22) | ||
| J | AT20G J | 0.677 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 1.86 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.659 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.525 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 1257 | 0.224 | Schwope+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | SDSS J | 1.14 | Gabány+ (2018) | bcu | FSRQ | 0 | SDSS. The 4FGL originally associated the gamma-ray source with 4C , which has a steep radio spectrum, and is likely a head-tail radio galaxy (MIS). However, a detailed analysis by Gabány+ (2018) showed that the most likely counterpart is the FSRQ SDSS J, which is from 4C . | ||
| J | RX J | 0.293 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 2.26 | Hook+ (1996) | fsrq | FSRQ | 0 | - | ||
| J | Cen A | 0.00183 | Lavaux+Hudson (2011) | RDG | MIS | 0 | FRI | ||
| J | 1RXS J | 0.458 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | LEDA 1410672 | 0.204 | Cao+ (1999) | bll | BLLAC | 0 | SDSS | ||
| J | TXS | 1.88 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | B2 | 1.40 | Hook+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 1.01 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 2MASS J | 0.236 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | 2E | 0.338 | Table A2 | bll | BLLAC | 1 | SDSS. Schwope+ (2000) reported an uncertain . | ||
| J | HE | 0.578 | Goldschmidt+ (1992) | bcu | FSRQ | 0 | No spectrum is published in Goldschmidt’s paper, but the redshift was later confirmed by Wisotski+ (2000) and 6dF | ||
| J | NVSS J | 0.343 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | 1RXS J | 0.438 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MG2 J | 0.731 | Table A2 | bll | BLLAC | 1 | Healey+ (2008). Dong+ (2018) reported from visual inspection of LAMOST DR2 & DR3 data, but there are no spectra available in the online database. SDSS gives on the basis of a discontinuity at Å identified as Ly, but the spectrum is very noisy, inconclusive. | ||
| J | 87GB | 0.688 | Healey+ (2008) | bcu | AMB | 0 | Healey classified it as NLRG. Shaw+ (2012) confirmed the redshift and noted the Ca H&K break plus a strong [OII] emission line. No broad lines found, so they favor the Healey’s classification. However, the radio spectrum is borderline () and no morphological studies were published. | ||
| J | 3C 286 | 0.850 | Lynds+ (1965) | css | MIS | 0 | SDSS. Radio morphology (CSS) An+ (2017). Optical spectrum NLS1 by Berton+ (2017). | ||
| J | RX J | 0.270 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.250 | Álvarez Crespo+ (2016) | bll | FSRQ | 0 | The published spectrum showed [OIII]>H, and a distorted H profile similar to [OIII]. Check for SEY/NLS1 classification. | ||
| J | TXS | 0.631 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.35 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.180 | Machalski+Condon (1999) | bcu | BLLAC | 0 | Machalski+Condon (1999) simply classified the radio source as AGN, without any other information. No spectrum published, no radio data except for NVSS. Shectman+ (1996) reported a slightly different , but perhaps is just the source at the center of the field. Peña-Herazo+ (2019) published a featureless spectrum, which implies a BLLAC classification. | ||
| J | PKS | 2.15 | Thompson+ (1990) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 0.669 | Landt+ (2001) | fsrq | FSRQ | 0 | SDSS. Landt+ (2001) also classified the source as SSRQ, but Specfind reported a flat radio spectrum ( 0.1–0.3). | ||
| J | PMN J | 1.49 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | 0.728 | SDSS | fsrq | CLAGN | 0 | Hook+ (1996) and Sowards-Emmerd+ (2005) reported featureless spectra, while Healey+ (2008) classified it as FSRQ with (no spectrum published), likely by identifying the line at Å as CIV. It seems that SDSS spectrum, although noisy, displays more lines and seems to be more reliable for the redshift measurement. It remains the CLAGN classification due to the first two featureless spectra, although the weakness of the lines and the noisy continuum might point to a lack of sufficient S/N. | ||
| J | CLASS J | 1.37 | Shaw+ (2009) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | TXS | 0.343 | Laurent-Muehleisen+ (1998) | fsrq | MIS | 0 | Laurent-Muehleisen+ (1998) also classified it as BLRG. Rafter+ (2011) classified it as FRI. | ||
| J | 1ES | 0.513 | Rector+ (2000) | bll | BLLAC | 0 | Stocke+ (1991) reported and strong spectral changes between two epochs (from strong emission lines to a featureless continuum). The coordinates reported by Stocke are from the position of 1ES : perhaps, there was a pointing error. | ||
| J | 2MASS J | 0.267 | SDSS | bll | BLLAC | 0 | - | ||
| J | S4 | 1.10 | Stickel+Kühr (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.539 | Wilkes (1986) | fsrq | FSRQ | 0 | Wilkes’ measurement based only on one line identified as MgII. Confirmed by Stickel+ (1993) | ||
| J | PMN J | 0.482 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.945 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | SDSS J | 0.771 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.657 | Hook+ (2003) | bcu | FSRQ | 0 | Confirmed by Rajagopal+ (2021). | ||
| J | PKS | 1.51 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.62 | Bolton+ (1970) | fsrq | FSRQ | 0 | 2dF | ||
| J | NVSS J | 0.246 | Smith+Spinrad (1980) | bcu | MIS | 0 | FRI, Laing+ (1983) | ||
| J | TXS | 2.26 | Falco+ (1998) | bcu | FSRQ | 0 | - | ||
| J | RX J | 0.546 | Beckmann+ (2003) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.223 | Paiano+ (2017) | bll | BLLAC | 0 | - | ||
| J | WN B | 0.761 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.171 | Bade+ (1996) | bll | AMB | 0 | SDSS. It is classified BL Lac Object, but Specfind reported a steep radio spectrum (). No information about the radio morphology. | ||
| J | SBS | 0.207 | Stepanian (2005) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 0.243 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 1.58 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.283 | SDSS | fsrq | BLLAC | 0 | - | ||
| J | 4C | 0.136 | Burbidge (1967) | bll | MIS | 0 | Burbidge reported no strong emission lines (only [OII] and Ca H&K break, no spectrum published). However, Grandi (1983) published a spectrum with broad and prominent emission lines ([OIII], H, H), and classified it as BLRG. The MIS classification (FRI-type) is confirmed by Gendre+Wall (2008) and the steep radio spectrum in Specfind (). Some doubts remain about the optical classification: Seyfert 1 by Grandi 1983, Lipovetsky+ (1988); Seyfert 2 by Thompson+ (1990); and it is also worth reminding the BL Lac-type spectrum reported by Burbidge. SDSS and LAMOST spectra suggest an intermediate Seyfert. There is the possibility of a rather odd CLAGN, with spectral changes determined both by the accretion and the partial covering. | ||
| J | 6C B | 0.932 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | GC | 1.35 | Xu+ (1994) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 2.51 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | B3 | 2.54 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | - | - | bll | UNCL | 3 | - | ||
| J | TXS | 1.09 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | - | - | bll | BLLAC | 2 | Ricci+ (2015) | ||
| J | NVSS J | 1.13 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.30 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.250 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.340 | Hewitt+Burbidge (1993) | fsrq | FSRQ | 0 | - | ||
| J | B2 B | 0.712 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS, apparent red-wing in the H profile. | ||
| J | PKS | 2.08 | Dunlop+ (1989) | fsrq | FSRQ | 0 | Radio structure unresolved according to Dunlop, but specfind gives a mildly steep radio spectrum () | ||
| J | RX J | 0.456 | Table A2 | bll | BLLAC | 1 | Sandrinelli+ (2013) | ||
| J | 2MASX J | 0.285 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | 87GB | 1.16 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.03 | Hook+ (2003) | bcu | BLLAC | 0 | Hook observed only one weak line, identified as MgII, in a noisy spectrum. Chu+ (1986) reported a featureless spectrum, likely due to an active jet. Specfind gives a mildly steep radio spectrum (). | ||
| J | PMN J | 1.30 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Featureless, Sbarufatti+ (2006). Many papers in the literature made a significant confusion with the nearby (∼) Seyfert 1 QSO at (see Veron 1996). | ||
| J | RGB J | 0.216 | Brinkmann+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | OP 186 | 0.752 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | RX J | 0.404 | SDSS | bll | BLLAC | 0 | The SDSS measurement is based on absorption features identified as G Band and Ca H+K. Bade+ (1998) measured on the basis of the same absorption features. It seems that Bade was misled by the noise around the Ca H+K feature. There is also a LAMOST spectrum, but it is too noisy and inconclusive, although slightly in favor of SDSS measurement. It would be better to confirm the SDSS value with a high S/N spectrum. | ||
| J | NVSS J | 0.358 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | 87GB | 1.03 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 3.72 | Dunlop+ (1986) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.492 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | NVSS J | 0.276 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.332 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | PKS B | 0.0747 | Jones+ (2009) | agn | MIS | 0 | Classified as FR0 by Glowaki+ (2017). | ||
| J | 4C | 0.720 | Burbidge+Kinman (1966) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.219 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | Spectrum not published, but confirmed independently by Anderson+Filipovic (2009), although also the latter was not published. | ||
| J | S5 | 1.58 | Shaw+ (2012) | fsrq | FSRQ | 0 | Shaw flagged the value as uncertain, because the spectrum is quite noisy and there is only one evident line at Å, identified as CIV. Another weak feature at Å is identified as MgII. Hook+ (1996) reported a featureless spectrum, but this is due to a smaller wavelength range (∼4800–9500 Å), which did not allow to detect the CIV, while MgII is too weak to emerge from the background noise. | ||
| J | NVSS J | 0.855 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 1.01 | Fabrika+ (2011) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 1.33 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | SDSS | ||
| J | 87GB | 0.407 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.334 | Shaw+ (2013) | bll | BLLAC | 0 | Ricci+ (2015) reported a featureless spectrum, likely due to an increased jet activity | ||
| J | 2MASS J | 0.203 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS B | 0.667 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.00 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 0.245 | Baldwin+ (1977) | bll | AMB | 0 | Baldwin recognized this BL Lac as very peculiar, having a significant extended radio emission. Further works (e.g., Hintzen+Owen 1981 and Saikia+ 1984) suggested it could be borderline between BL Lac and FRI classes (specfind gives ). SDSS spectrum displays strong and narrow emission lines, confirming a large viewing angle or, at least, a partial covering. H emission line is almost absent in LAMOST spectra (1; 2), although these spectra a much more noisy. | ||
| J | PMN J | 2.14 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | MS | 0.920 | Table A2 | bll | BLLAC | 1 | Observed many times, but almost always showing a featureless spectrum. An early uncertain was proposed by Perlman+ (1996), but neither the spectrum was published, nor any other indication of how it was measured. Falomo+Kotilainen (1999) wrote that this value is not in disagreement with the imaging of the host galaxy (unresolved). Bauer+ (2000) reported , but no indication of how it was measured. SDSS inconclusive, although there is an emission feature at ∼5700–5800 Å: if Bauer’s value is correct (), then the feature might be the H-[OIII] complex, and would be consistent with the identification of the break at Å with the absorption of the host galaxy (Ca H+K). | ||
| J | NVSS J | 0.363 | Bade+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.640 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | NVSS J | 0.420 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Piranomonte+ (2007) | ||
| J | RBS 1350 | 0.339 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007) | ||
| J | ESO | 0.0242 | Smith+ (2000) | bll | BLLAC | 0 | 6dF. This seems to be a rare case of BL Lac Object in a S0 host galaxy. | ||
| J | SUMSS J | - | - | bll | BLLAC | 2 | Featureless. Klindt+ (2017) proposed a tentative based on rather doubtful absorption features. | ||
| J | PKS B | 1.49 | Peterson+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.24 | Table A2 | bll | BLLAC | 1 | Featureless, Sbarufatti+ (2009). SDSS inconclusive (although, a triple emission feature at ∼8300–8500 Å might be the H-[OIII] complex, which would imply ). | ||
| J | NVSS J | 0.144 | SDSS | bll | BLLAC | 0 | - | ||
| J | RX J | 0.383 | Bade+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | RX J | 0.521 | SDSS | bll | BLLAC | 0 | - | ||
| J | TXS | 0.582 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.283 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | SBS | 0.0760 | Stepanian (2005) | bll | MIS | 0 | Steep radio spectrum, classified as FR0 by Miraghei+Best (2017). SDSS | ||
| J | FIRST J | 0.948 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.542 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | SDSS J | 1.53 | SDSS | bcu | FSRQ | 0 | - | ||
| J | RX J | 0.496 | SDSS | bll | BLLAC | 0 | Although the spectrum is rather noisy, the redshift is consistent with the estimate () from the imaging of the host galaxy by Nilsson+ (2003) | ||
| J | PKS B | 2.00 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PKS B | 0.334 | Table A2 | bcu | AMB | 1 | It seems that the jetted AGN is behind a Seyfert 2 galaxy at (SDSS). See detailed analyses in Stocke+ (1992), Perlman+ (2002), and Readhead+ (2021) | ||
| J | NVSS J | 0.136 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | 1E | 0.236 | Halpern+ (1986) | bll | BLLAC | 0 | Halpern also suggested that the host galaxy could be a spiral, but subsequent analyses favored the elliptical host (Romanishin 1992, Gladders+ 1997). SDSS image also shows a nearby galaxy at the same z: an incoming merger? | ||
| J | 4C | 1.56 | Walsh+ (1979) | fsrq | FSRQ | 0 | SDSS | ||
| J | 87GB | 0.819 | Peña-Herazo+ (2021) | BCU | FSRQ | 0 | SDSS automatic measurement gives a wrong result (), because it identifies the apparent MgII emission line at Å as Ly, which is obviously not the case. | ||
| J | NVSS J | 0.075 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | PKS | 1.54 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.014 | Masetti+ (2013) | bll | BLLAC | 0 | - | ||
| J | 2MASS J | 0.809 | Table A2 | bll | AMB | 1 | Classified as Broad-Absorption Line (BAL) QSO at by Trump+ (2006) on the basis of SDSS-DR3. Latest SDSS spectrum is noisy and inconclusive. Radio detections only at GHz. | ||
| J | NVSS J | 0.903 | Buckley+ (2015) | fsrq | FSRQ | 0 | - | ||
| J | B3 | 1.83 | Lahulla+ (1991) | fsrq | FSRQ | 0 | SDSS | ||
| J | OQ 530 | 0.152 | Stickel+ (1993) | bll | BLLAC | 0 | SDSS. Host galaxy classified as S0 by Wurtz+ (1996). Another rare case of BL Lac Object in a S0 host galaxy. | ||
| J | SDSS J | 0.625 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | TXS | 0.489 | White+ (2000) | fsrq | FSRQ | 0 | SDSS. The source was classified as NLS1 by Rakshit+ (2017) on the basis of the SDSS spectrum, which in turn displays an apparent artifact affecting half of the H profile. Rakshit himself changed into FSRQ the classification of the source in 2020 (Rakshit+ 2020). White’s paper shows a complete spectrum, where the broad profile of H is evident. | ||
| J | PMN J | 1.17 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 1.85 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | OQ 334 | 0.682 | Wills+Wills (1974) | fsrq | CLAGN | 0 | SDSS. Classified as CLAGN by Mishra+ (2021) | ||
| J | 1ES | 0.636 | Bade+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.454 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 87GB | 0.749 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | PKS | 0.788 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.368 | Table A2 | bcu | BLLAC | 1 | LAMOST | ||
| J | NVSS J | 0.0823 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | TXS | 0.452 | Table A2 | bll | BLLAC | 1 | Chavushyan+ (2001). | ||
| J | SDSS J | 0.557 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | FBQS J | 0.47 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 2QZ J | 0.511 | Table A2 | bll | BLLAC | 1 | SDSS. Londish+ (2002) reported , but this value was never confirmed by Croom+ (2004) and Londish+ (2007) | ||
| J | RGB J | 0.488 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | B2 | 1.09 | Henstock+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.605 | Paiano+ (2017) | BLL | BLLAC | 0 | - | ||
| J | NVSS J | 0.678 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.404 | Table A2 | bll | BLLAC | 1 | Titov+ (2013) | ||
| J | NVSS J | 0.208 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.52 | White+ (1988) | FSRQ | FSRQ | 0 | - | ||
| J | MG1 J | 0.560 | Smith+ (2018) | bcu | FSRQ | 0 | Spectra (ESO NTT + P60) | ||
| J | 87GB | 2.13 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | H | 0.129 | Remillard+ (1989) | bll | BLLAC | 0 | SDSS | ||
| J | 1RXS J | 1.233 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.245 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 3.01 | Henstock+ (1997) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.265 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.150 | Table A2 | bll | UNCL | 1 | - | ||
| J | GALEXASC J | 0.839 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.33 | Wright+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.200 | Desai+ (2019) | bcu | BLLAC | 0 | - | ||
| J | B3 | 1.24 | Vermeulen+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | OQ 253 | 1.38 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | LAMOST | ||
| J | 1RXS J | 0.574 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | TXS | 0.748 | Shaw+ (2013) | bll | MIS | 0 | SDSS clearly shows only strong and narrow emission lines—confirmed by the FWHM measured by Rakshit+ (2020)—suggesting the view at large angles, hypothesis strengthened by a steep radio spectrum (). | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS B | 1.55 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | RBS 1409 | 0.15 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.29 | Jauncey+ (1982) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.848 | SDSS | bll | BLLAC | 0 | - | ||
| J | B2 B | 2.40 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | PG | 0.344 | Piranomonte+ (2007) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.160 | Desai+ (2019) | bcu | BLLAC | 0 | - | ||
| J | GB6 J | 0.174 | Falco+ (1998) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.300 | Marchesini+ (2019) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.702 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | 0.309 | Paiano+ (2021) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.141 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | PMN J | 0.396 | Sandrinelli+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 2.64 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.624 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | SDSS J | 0.550 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SDSS J | 0.698 | Pursimo+ (2013) | bcu | FSRQ | 0 | - | ||
| J | SUMSS J | 0.103 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | 1ES | 0.163 | Schachter+ (1993) | bll | BLLAC | 0 | SDSS. The AGN has two close companions: one is a foreground star, the other is another galaxy at the same redshift, likely interacting. See Sbarufatti+ (2006) and references therein. | ||
| J | B3 | 0.703 | Yuan+ (2008) | nlsy1 | NLS1 | 0 | SDSS. Early classifications indicated a steep radio spectrum, but recent observations measured a flat spectrum, suggesting that the steepness was due to non-simultaneous observations. See Berton+ (2018) and references therein. | ||
| J | 3C 303 | 0.141 | Spinrad (1976) | rdg | MIS | 0 | SDSS. Classified as FRII by Laing+ (1983). Optical spectrum: Seyfert intermediate | ||
| J | NVSS J | 0.529 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.940 | Shaw+ (2012) | fsrq | FSRQ | 0 | Shaw reported FWHM(H) km/s, but the published spectrum is quite noisy in the red part, where H should be. The SDSS spectrum is a bit better and clearly shows the H-[OIII] complex. The H profile is distorted, with an apparent red wing. The analysis by Rakshit+ (2020) resulted in a slightly greater FWHM ( km/s), but still in the NLS1 range. This source was detected MAGIC at VHE in 2015 Ahnen+ (2015), and, therefore, it might be the first NLS1 detected at VHE. However, the reanalysis of SDSS spectrum by one of us (S.C.) rejected the NLS1 classification and confirmed that as FSRQ. | ||
| J | PKS | 0.139 | Goldoni+ (2021) | bll | BLLAC | 0 | - | ||
| J | RBS 1424 | 0.119 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | PKS B | 0.989 | Table A2 | bll | BLLAC | 1 | Titov+ (2011) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.079 | Table A2 | bcu | BLLAC | 1 | Truebenbach+Darling (2017) | ||
| J | S3 | 1.02 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS. Sowards-Emmerd+ (2005) reported : perhaps a typo? | ||
| J | NVSS J | 0.814 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.331 | Paiano+ (2021) | bcu | BLLAC | 0 | - | ||
| J | RBS 1432 | 0.449 | Table A2 | bll | BLLAC | 1 | Paiano+ (2020) | ||
| J | B2 | 0.0307 | Huchra+ (1990) | rdg | MIS | 0 | Classified as FRI by Angioni (2020), S0 host galaxy. | ||
| J | PKS B | 0.938 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.159 | Table A2 | agn | UNCL | 1 | - | ||
| J | TXS | 2.63 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | SDSS J | 2.47 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS. The redshift was measured on the basis of the Ly forest, although Paiano+ (2017) suggest it is only a lower limit. This seems to be the farthest BL Lac Object. | ||
| J | RX J | 0.650 | Bade+ (1998) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.529 | SDSS | bcu | MIS | 0 | There are no publications on either the radio morphology or the spectrum (just the NVSS detection), but the optical spectrum is typical of Type 2 AGN. | ||
| J | PKS | 0.204 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.715 | Healey+ (2008) | fsrq | BLLAC | 0 | Hook+ (1998) reported a featureless spectrum with Lick 3 m telescope in 1995. It is worth noting that the SDSS spectrum (taken in 2011) displays weak emission lines, and Rakshit+ (2020) measured EW just a little bit above the 5 Å threshold. Rakshit also measured FWHM(H) = km/s, suggesting a NLS1 classification, but the weakness of the lines suggests that the narrowness might be due to the jet activity (cf Foschini 2012). Further observations are required. | ||
| J | 87GB | 2.11 | SDSS | bcu | FSRQ | 0 | - | ||
| J | CLASS J | 1.27 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | B2 | 0.757 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | TXS | 1.08 | Stepanian (2005) | bll | BLLAC | 0 | Paiano+ (2020) reported a featureless spectrum, likely due to the increased jet activity. | ||
| J | PKS | 0.314 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | 87GB | 0.522 | Table A2 | bll | BLLAC | 1 | Sandrinelli+ (2013) | ||
| J | PKS | 0.095 | Hook+ (2003) | bcu | MIS | 0 | Steep radio spectrum, likely a FRI (cf Jones+McAdam 1992). | ||
| J | SUMSS J | - | - | bcu | BLLAC | 2 | Rajagopal+ (2021) | ||
| J | RGB J | 0.480 | Bade+ (1998) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.358 | Table A2 | bcu | UNCL | 1 | Typo in the 4FGL name: it is written PKS J, but the coordinates are clearly referred to B1950, not J2000. | ||
| J | PKS | 1.42 | Hook+ (2003) | FSRQ | FSRQ | 0 | - | ||
| J | PMN J | 0.112 | Goldoni+ (2021) | bcu | BLLAC | 0 | - | ||
| J | B3 | 0.333 | Vermeulen+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | SDSS J | 0.672 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum (): MIS? | ||
| J | 3C | 0.905 | Burbidge+Kinman (1966) | css | MIS | 0 | Classified as CSS by van Breugel+ (1984) with a viewing angle Wilkinson+ (1986) | ||
| J | MG1 J | 0.370 | SDSS | fsrq | BLLAC | 0 | - | ||
| J | TXS | 1.06 | Britzen+ (2008) | bll | BLLAC | 0 | - | ||
| J | FIRST J | 0.503 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MS | 0.235 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | FIRST J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.674 | Table A2 | bll | UNCL | 1 | - | ||
| J | TXS | 0.344 | SDSS | bll | MIS | 0 | Steep radio spectrum, core dominance (Brotherton+ 2015), type 2 optical spectrum. | ||
| J | RBS 1457 | - | - | bll | BLLAC | 2 | Paiano+ (2020) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 1.84 | Smith+ (1977) | FSRQ | FSRQ | 0 | Previous reports by Burbidge+Strittmatter (1972) suggested . SDSS | ||
| J | PKS | 0.408 | Wills+Lynds (1978) | NLSY1 | NLS1 | - | Classified as NLS1 by Zhou+ (2006). SDSS | ||
| J | PMN J | 0.359 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | WISEA J | 0.329 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.673 | Stickel+Kühr (1994) | fsrq | FSRQ | - | SDSS, Type 2 optical spectrum, but flat radio spectrum. Likely jet-cloud interaction Wiklind+Combes (1996), Carilli+ (1997), Kanekar+Chengalur (2008) | ||
| J | NVSS J | 0.470 | SDSS | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.518 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.592 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.565 | SDSS | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.206 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.248 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 1467 | 0.270 | Beckmann+ (2003) | bll | BLLAC | 0 | SDSS. Spiral galaxy of unknown redshift at | ||
| J | PMN J | 0.776 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | SBS | 0.578 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | AT20G J | - | - | bcu | UNCL | 3 | - | ||
| J | GB | 4.31 | Hook+ (1995) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.868 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.19 | Peterson+Bolton (1972) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.907 | Table A2 | bll | BLLAC | 1 | Goldoni+ (2021) | ||
| J | 1RXS J | 0.315 | Böhringer+ (2004) | bll | BLLAC | 0 | Marchesini+ (2016) reported a featureless spectrum, likely due to an increased jet activity. | ||
| J | PKS | 0.220 | Savage+ (1976) | fsrq | MIS | 0 | SDSS, type 2 optical spectrum. Steep radio spectrum (). | ||
| J | B3 | 1.14 | Garnett+ (2017) | bcu | BLLAC | 0 | SDSS quite noisy, but there is a clear emission feature at Å consistent with the identification as MgII. | ||
| J | PKS | 0.360 | Burbidge+Kinman (1966) | FSRQ | FSRQ | 0 | Optical spectrum Torrealba+ (2012) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.149 | Table A2 | bll | BLLAC | 1 | 6dF: the main feature at Å might be MgII: then | ||
| J | PKS | 1.15 | Ackermann+ (2011) | fsrq | FSRQ | 0 | Optical follow-up program of the Fermi LAT collaboration, but no more info available and no paper was published. | ||
| J | 2MASS J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | - | - | bcu | BLLAC | 2 | 6dF: one absorption feature at Å might be Ca H+K break: then | ||
| J | PMN J | 0.348 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 1.12 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | PKS | 0.053 | Searle+Bolton (1968) | rdg | MIS | 0 | SDSS. Classified as FRII by Fanaroff+ (2021) | ||
| J | RGB J | 0.130 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | MG2 J | 0.814 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.07 | Persic+Salucci (1986) | bll | BLLAC | 0 | SDSS spectrum is noisy, but it confirms the broad emission feature at Å, which is consistent with MgII. Many other featureless observations are reported in the literature, likely due to a higher activity of the jet (Shaw+ 2013 observation was made on the source with optical flux greater than Persic+Salucci’s by a factor ); Sowards-Emmerd+ (2005) reported from archives, but no further information is available (it was likely from Snellen+ 2002, which was a photometric z). | ||
| J | SDSS J | 0.549 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.819 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1H | 0.738 | Table A2 | bll | BLLAC | 1 | Beckmann+ (1999) reported on the basis of some absorption features; although it is a lower limit, it was often taken as a firm value in the literature. None of the more recent observations confirmed it, last one Shaw+ (2013). Scarpa+ (1999) reported arc-like features surrounding the point source in the HST images, suggesting gravitational lensing, which was later excluded by O’Dowd+ (2005). These features seem to be the residual of a merger. | ||
| J | AP Librae | - | 0.0490 | Disney+ (1974) | bll | BLLAC | 0 | 6dF | |
| J | TXS | 0.128 | Becerra González+ (2021) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.642 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | TXS | 0.102 | Owen+ (1995) | rdg | MIS | 0 | SDSS. Classified as Narrow-Angle Tail FRI by O’Dea+ (1987) and Miraghei+Best (2017) | ||
| J | GB6 J | 0.065 | Laurent-Muehleisen+ (1998) | bll | AMB | 0 | SDSS. Laurent-Muehleisen classified it as Seyfert 1, measuring FWHM(H) km/s. However, H is almost absent, and there are strong oxygen narrow lines, suggesting some obscuration and, hence, a large viewing angle. It seems a Seyfert 1.9, Singha+ (2021) classified it as LERG with outflows, but the radio spectrum is flat. | ||
| J | 1RXS J | 0.902 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.480 | Table A2 | bll | BLLAC | 1 | SDSS: there is a feature at Å: if MgII, then | ||
| J | B3 | 0.485 | Shaw+ (2012) | fsrq | AMB | 0 | SDSS. Classified NLS1 by Rakshit+ (2017) with FWHM(H) km/s, but Rakshit+ (2020) reported FWHM(H) km/s. SDSS image shows a distorted point source: contaminating source? on-going merging? | ||
| J | NVSS J | 1.00 | Table A2 | bll | BLLAC | 1 | Goldoni+ (2021) | ||
| J | PKS B | 0.052 | Drinkwater+ (1997) | rdg | MIS | 0 | SDSS. Classified FRI by Miraghei+Best (2017) | ||
| J | B3 | 2.17 | Hook+ (1996) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 | 1.49 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 1.29 | Heidt+ (2004) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.799 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GALEXASC J | 0.587 | Table A2 | bll | BLLAC | 1 | Paiano+ (2019) | ||
| J | 2MASX J | 0.214 | Table A2 | bcu | BLLAC | 1 | 6dF | ||
| J | B2 | 1.39 | Barbieri+ (1975) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.833 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.831 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | WN B | 1.05 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | WN B | 0.723 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | SDSS J | 1.04 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | RX J | 0.0650 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | TXS | 0.707 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.307 | Piranomonte+ (2007) | bll | BLLAC | 0 | SDSS | ||
| J | RX J | 0.981 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 1.43 | Wampler+ (1984) | fsrq | FSRQ | 0 | SDSS | ||
| J | RGB J | 0.143 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | SDSS | ||
| J | 1ES | 0.890 | Bade+ (1998) | bll | BLLAC | 0 | - | ||
| J | 2MASS J | 0.253 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.257 | White+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | - | - | bll | BLLAC | 2 | Titov+ (2011) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.984 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG2 J | 2.20 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.837 | Table A2 | bll | BLLAC | 1 | Goldoni+ (2021) | ||
| J | 87GB | 0.808 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1ES | 0.227 | Table A2 | bll | BLLAC | 1 | Paiano+ (2017) | ||
| J | CRATES J | 0.693 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 0.606 | Stickel+ (1993) | bll | BLLAC | 0 | SDSS | ||
| J | WISE J | 0.223 | Paiano+ (2019) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 1.40 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | OR 167 | 1.66 | Wills+Wills (1976) | fsrq | MIS | 0 | SDSS. Steep radio spectrum, likely an unresolved FRII according to Gendre+ (2008) | ||
| J | GB6 J | 0.528 | Table A2 | bll | BLLAC | 1 | Marchã+Caccianiga (2013) reported a tentative , but it was not confirmed in subsequent papers. | ||
| J | CGCG | 0.0400 | Karachentseva+ (1988) | agn | BLLAC | 0 | - | ||
| J | NVSS J | 0.171 | Chornock+Margutti (2017) | bcu | BLLAC | 0 | - | ||
| J | NVSS J | 0.121 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | RX J | 1.06 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 1.34 | Table A2 | bll | UNCL | 1 | - | ||
| J | MG1 J | 0.538 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.876 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.231 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.461 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.192 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.588 | Table A2 | bcu | BLLAC | 1 | Hook+ (1996) | ||
| J | SDSS J | 0.799 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | WN B | 1.25 | Table A2 | bll | UNCL | 1 | - | ||
| J | WB J | 0.342 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.414 | Burbidge+Strittmatter (1972) | fsrq | FSRQ | 0 | SDSS | ||
| J | MG1 J | 1.20 | Caccianiga+ (2019) | bll | BLLAC | 0 | SDSS noisy; see Footnote 2 in Caccianiga+ (2019) | ||
| J | NVSS J | 0.418 | Paiano+ (2020) | bll | BLLAC | 0 | - | ||
| J | NVSS J | - | - | bcu | BLLAC | 2 | Rajagopal+ (2021) | ||
| J | 4C | 1.42 | White+ (1988) | fsrq | FSRQ | 0 | SDSS | ||
| J | 4C | 0.937 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum. Stickel+Kühr (1996) classified it as QSO, but neither spectrum information nor redshift was given | ||
| J | NVSS J | 0.284 | Table A2 | bll | UNCL | 1 | - | ||
| J | TXS | 1.31 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.608 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013). Peña-Herazo+ (2021) reported on the basis of a LAMOST spectrum released with the DR5. However, the spectrum is no more present in DR7. | ||
| J | NVSS J | 0.485 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | 0.0839 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015). Masetti+ (2013) suggested a tentative on the basis of a weak feature identified as H | ||
| J | PKS | 1.31 | Cristiani+Koehler (1987) | fsrq | FSRQ | 0 | SDSS. Savage+Wright (1981) proposed | ||
| J | PKS | 0.332 | Shaw+ (2012) | fsrq | SEY | 0 | Classified as LINER by Shaw+ (2012) | ||
| J | GALEXASC J | 0.625 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.541 | Table A2 | bll | BLLAC | 1 | SDSS: there are two emission features, which seem to be consistent with : Å for [OIII], Å for [OII] | ||
| J | PG | 0.028 | Table A2 | BLL | BLLAC | 1 | This BL Lac Object has a very long record of attempts to determine the redshift, but today there is no consensus yet. Miller+Green (1983) reported on the basis of a IUE spectrum and two features identified as Ly and NV, but in a subsequent work (Miller+ 1988), they did not confirm this measurement. A reanalysis of IUE data by Falomo+Treves (1990) did not confirm the presence of these features. Later, the IUE calibrated spectrum was published, showing a prominent Ly (Kinney+ 1991), but being at the extreme low wavelength end of the spectrum, it might be an artifact. More recent observations by HST/COS did not detect any emission features (Danforth+ 2010). Monroe+ (2016) display a GALEX spectrum, rather noisy, but with a broad and unknown feature at Å. Abramowski+ (2015) suggested on the basis of the extragalactic background absorption of very-high energy gamma rays. Sometimes, the value is still adopted, perhaps it is consistent with other estimates of lower/upper limits; sometimes, no value is given. | ||
| J | PKS | - | - | bll | UNCL | 3 | - | ||
| J | PKS | 1.77 | Baldwin+ (1981) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.0974 | Peterson+ (1979) | fsrq | SEY | 0 | 6dF | ||
| J | TXS | 0.397 | Table A2 | bll | BLLAC | 1 | SDSS. Falco+ (1998) reported on the basis of the detection of absorption features of the host galaxy (Ca H+K, G) and H. However, more recent observations by Shaw+ (2013) with greater S/N and jet at the lowest activity, never confirmed these detections. | ||
| J | NVSS J | 0.581 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.416 | Marchesini+ (2019) | bcu | BLLAC | 0 | - | ||
| J | 87GB | 0.673 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | WN B | 0.986 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.10 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OS 300 | 1.1 | Snellen+ (2000) | bcu | MIS | 1 | Classified as CSS/GPS by O’Dea (1998). Many redshift estimates, but none reliable: Wills+Wills (1976) classified it as a star on the basis of absorption features identified as Ca H+K; Wall+Peacock (1985) reported a tentative , on the basis of personal communications from colleagues; O’Dea (1998) set for sources with unknown redshift. | ||
| J | RGB J | 0.860 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | MG1 J | 0.143 | Healey+ (2008) | bll | BLLAC | 0 | - | ||
| J | SDSS J | 0.470 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | GB6 J | 0.722 | Falco+ (1998) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.674 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | TXS | 1.05 | Table A2 | bcu | BLLAC | 1 | Desai+ (2019) reported the detection of a weak emission feature at Å: if [OII], then ; if [OIII], then . The former might be consistent with another weak feature at Å identified as H | ||
| J | RBS 1555 | 0.212 | Rowan-Robinson+ (2004) | bll | BLLAC | 0 | SDSS. The host is classified as spiral by Rowan-Robinson+ (2004) | ||
| J | RX J | - | - | bcu | AMB | 3 | The X-ray source is associated at a galaxy cluster with (Böhringer+ 2000). It is likely that the ray emission is due to the brightest radio source, but there is only one found within from the counterpart coordinates of the 4FGL: NVSS J at . However, no information are available on this source, except for the NVSS detection | ||
| J | MG1 J | 0.290 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | SDSS | ||
| J | RBS 1558 | 0.437 | Schwope+ (2000) | bll | SEY | 0 | SDSS | ||
| J | B2 | 0.933 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | 4C | 0.496 | Shaw+ (2012) | bll | BLLAC | 0 | The SDSS spectrum is so noisy that the automatic pipeline failed. At Å there is the H-[OIII] complex consistent with Shaw’s redshift, which was not recognized. Warning: NED associated this source with 3EG J, for which Sowards-Emmerd+ (2003) proposed the counterpart to be J, a FSRQ at . However, this source is far from 4C . Maybe there was an error in the epoch of coordinates (4C is J = B to be compared with J). | ||
| J | NVSS J | - | - | bll | UNCL | 3 | - | ||
| J | B2 | 0.628 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | 4C | 1.23 | Stickel+Kühr (1994) | fsrq | FSRQ | 0 | SDSS | ||
| J | B2 | 1.45 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.1 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.0296 | Jones+ (2009) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.9 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | 2MASS J | 0.632 | Table A2 | bcu | UNCL | 1 | - | ||
| J | OS 319 | 1.40 | Burbidge (1970) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.344 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 1.63 | SDSS | bcu | FSRQ | 0 | - | ||
| J | B3 | 0.199 | SDSS | fsrq | MIS | 0 | Classified FRI by Miraghei+Best (2017) | ||
| J | MG4 J | 0.950 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.572 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B3 | 0.267 | White+ (2000) | bll | BLLAC | 0 | SDSS | ||
| J | PMN J | 1.81 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.1 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.71 | Hunstead+Murdoch (1980) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 2.56 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.520 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | 6C B | 0.527 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.0625 | Table A2 | bll | UNCL | 1 | - | ||
| J | 87GB | 0.464 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | SDSS J | 0.533 | SDSS | bcu | BLLAC | 0 | - | ||
| J | TXS | 0.789 | Vermeulen+ (1996) | fsrq | CLAGN | 0 | Vermeulen measured some emission lines from a spectrum taken on 1995 June, while Hook+ (1996) reported a featureless spectrum taken on 1992 April | ||
| J | SBS | 0.64 | Meisner+Romani (2010) | bll | BLLAC | 1 | - | ||
| J | 4C | 2.55 | Pearson+Readhead (1988) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.786 | di Serego Alighieri+ (1994) | fsrq | FSRQ | 0 | An early tentative was proposed by Wall+Peacock (1985), but never confirmed. | ||
| J | PKS B | 0.815 | Wright+Otrupcek (1999) | FSRQ | FSRQ | 0 | Caveat: There is neither the spectrum nor any other information published. Curiously, none took a new spectrum after that report. Still to date, this is the only redshift available. | ||
| J | RGB J | 0.498 | Kock+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.105 | Ricci+ (2015) | bll | BLLAC | 0 | - | ||
| J | MG4 J | 1.05 | Brinkmann+ (2000) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.580 | SDSS | bll | BLLAC | 0 | - | ||
| J | MG4 J | 2.33 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | CLASS J | 0.472 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | 6C B | 0.410 | Table A2 | bll | BLLAC | 1 | Hook+ (1996) | ||
| J | NGC 6251 | 0.0230 | Waggett+ (1977) | rdg | MIS | 0 | FRI. Waggett cited a personal communication for the redshift. The first optical spectrum is displayed in Miley+Osterbrock (1979). The counterpart coordinates in the 4FGL refer to the radio source marked as B3 in Mukherjee+ (2002), which was identified as the jet of NGC 6251. This radio source is from the VLBI core of the radio galaxy. | ||
| J | TXS | 0.492 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | MG1 J | 0.866 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.518 | Hook+ (1996) | fsrq | SEY | 0 | SDSS | ||
| J | 1RXS J | 0.234 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.26 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 1.81 | Strittmatter+ (1974) | FSRQ | FSRQ | 0 | SDSS | ||
| J | MG2 J | 0.520 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | MG3 J | 3.65 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | 7C | 0.171 | Appenzeller+ (1998) | bcu | FSRQ | 0 | - | ||
| J | NVSS J | 0.174 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.44 | Table A2 | bll | BLLAC | 1 | SDSS: if the feature at Å is CIV, and that at Å is OIII, then | ||
| J | 1RXS J | 0.656 | Sandrinelli+ (2013) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.343 | SDSS | bll | BLLAC | 0 | - | ||
| J | B3 | 0.192 | SDSS | bll | BLLAC | 0 | - | ||
| J | 4C | 0.735 | Walsh+Carswell (1982) | fsrq | FSRQ | 0 | SDSS | ||
| J | RX J | 0.892 | Table A2 | bll | BLLAC | 1 | Appenzeller+ (1998) | ||
| J | OS 562 | 0.751 | Walsh+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | MG4 J | 0.691 | SDSS | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.437 | Table A2 | bcu | BLLAC | 1 | Desai+ (2019) | ||
| J | NVSS J | 0.715 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NRAO 512 | 1.67 | Stickel+Kühr (1989) | FSRQ | FSRQ | 0 | SDSS | ||
| J | TXS | 0.0799 | Mitton+ (1977) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.718 | Table A2 | bll | BLLAC | 1 | Sowards-Emmerd+ (2004) reported an uncertain measured on a spectrum taken at HET on 2003 April or June (no exact date is given). However, Shaw+ (2013) reported no features on a spectrum taken at HET on MJD 52756 (2003 April 27). It seems to be a reanalysis of the same spectrum. | ||
| J | PKS | - | - | bll | BLLAC | 2 | Titov+ (2011) | ||
| J | 1RXS J | 0.592 | SDSS | bll | BLLAC | 0 | - | ||
| J | 3C 345 | 0.593 | Burbidge (1965) | FSRQ | FSRQ | 0 | SDSS | ||
| J | NVSS J | 1.42 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.0427 | Simpson+ (1993) | bll | MIS | 0 | Classified as FRII by Morganti+ (1993) | ||
| J | NVSS J | 0.0820 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.492 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | B3 | 0.225 | Kock+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | MG2 J | 0.144 | Bade+ (1995) | NLSY1 | NLS1 | 0 | SDSS. Classified NLS1 by Véron-Cetty+Véron (2001) | ||
| J | TXS | 2.38 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.187 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 7C | 0.920 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.3 | Table A2 | bcu | UNCL | 1 | Ultra steep radio spectrum (), De Breuck+ (2000), likely MIS | ||
| J | PMN J | 0.359 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | B2 | 0.133 | Marchã+ (1996) | bll | BLLAC | 0 | SDSS | ||
| J | SBS | 0.0490 | Marchã+ (1996) | bll | SEY | 0 | S0 host galaxy. In 2009, a SNII exploded in the host galaxy (2009fe; see, for example, fig. 15 in Hakobyan+ 2012) | ||
| J | MG2 J | 0.823 | SDSS | bcu | BLLAC | 0 | - | ||
| J | NVSS J | 2.5 | Schmidt+ (2006) | bcu | FSRQ | 1 | Schmidt classified it as Extremely Red Object (ERO): obscuration? | ||
| J | 87GB | 0.291 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | PKS | 0.711 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 1.97 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.113 | Table A2 | bll | BLLAC | 1 | Appenzeller+ (1998) | ||
| J | RX J | 0.669 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | Mkn 501 | 0.0335 | Wills+Wills (1974) | BLL | BLLAC | 0 | - | ||
| J | MG2 J | 1.08 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | bll | BLLAC | 2 | 6dF | ||
| J | RGB J | 0.623 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | 4C | 1.67 | Ackermann+ (2011) | fsrq | CLAGN | 0 | The optical follow-up should have been published in other papers, but none was found. Previous observations found a featureless spectrum (Healey+ 2008) or did not detect any object (Hook+ 1996) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | Titov+ (2017) took a low S/N spectrum; no information available | ||
| J | NVSS J | 0.374 | SDSS | bll | BLLAC | 0 | - | ||
| J | 4C | 0.795 | Wills+Wills (1974) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.301 | Henstock+ (1997) | fsrq | NLS1 | 0 | Henstock measured FWHM(H) km/s | ||
| J | 7C | 0.795 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.507 | Healey+ (2008) | bll | BLLAC | 0 | SDSS. Curiously, SDSS automatic pipeline measured the redshift correctly until DR7, but it failed in more recent releases, although the spectrum displays features (Ca H+K, [OII], [OIII]) consistent with Healey’s measurement | ||
| J | MG2 J | 0.632 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | RX J | 0.701 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MRC | 1.75 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.592 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.452 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 1.26 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2020) | ||
| J | GB6 J | 0.350 | Nilsson+ (2003) | bll | BLLAC | 1 | - | ||
| J | 1RXS J | - | - | bll | UNCL | 3 | The X-ray source corresponds to a galaxy cluster at (Kocevski+ 2007). No radio counterpart is found around 1 arcmin from the X-ray centroid | ||
| J | NVSS J | 0.345 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 0.645 | Walsh+ (1979) | fsrq | FSRQ | 0 | SDSS | ||
| J | MG1 J | 0.291 | de Menezes+ (2020) | fsrq | SEY | 0 | Only strong forbidden oxygen lines | ||
| J | NVSS J | 0.841 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 1.03 | Healey+ (2008) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | - | - | bcu | UNCL | 3 | Steep radio spectrum () | ||
| J | RX J | 0.304 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | NVSS J | 0.624 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.310 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B2 | 0.358 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | Hook+ (1996) reported a noisy spectrum and no redshift measured, but there is a feature at Å, which is consistent with [OIII] at 5007 Å. | ||
| J | S4 | 0.339 | Britzen+ (2008) | fsrq | FSRQ | 0 | Hewitt+Burbidge (1993) reported measured by Kühr (1980, PhD thesis) on the basis of one single feature identified as MgII. Stickel+Kühr (1994) adjusted the value to , but Britzen+ (2008) took a new better spectrum with many lines (H, H, [OII], [OIII]) and measured | ||
| J | PKS | 0.157 | Table A2 | bcu | BLLAC | 1 | Titov+ (2017) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.059 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.137 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | - | ||
| J | 87GB | 0.407 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 0.454 | SDSS | bcu | AMB | 0 | The SDSS spectrum seems a Seyfert 1.9; radio spectrum is steep (). Likely a SEY or MIS | ||
| J | GB6 J | 2.06 | Sowards-Emmerd+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.732 | Afanas’ev+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | B2 | 0.548 | SDSS | fsrq | SEY | 0 | Hewitt+Burbidge (1993) reported from a personal communication by Wills+ (1979): it seems that they have misidentified the emission line at Å with CIV instead of MgII. The SDSS spectrum shows a weak H and prominent oxygen lines, suggesting an obscured object, but the radio spectrum is flat. | ||
| J | S4 | 1.05 | Vermeulen+ (1996) | fsrq | BLLAC | 0 | Henstock+ (1997) reported a featureless spectrum, likely due to the jet activity | ||
| J | NGC 6328 | 0.0145 | Forbes+ (1977) | rdg | MIS | 0 | CSO/GPS very young FRII, SA host galaxy, Angioni+ (2019) | ||
| J | S5 | 0.680 | Stickel+Kühr (1994) | fsrq | FSRQ | 0 | No [OIII] lines | ||
| J | 1H | 0.028 | Table A2 | bll | BLLAC | 1 | Griffiths+ (1989) published an optical spectrum with two strong absorption features suggesting . However, the unresolved host galaxy suggests a greater value (e.g., Sbarufatti+ 2006 set ) | ||
| J | RX J | 0.061 | SDSS | bcu | BLLAC | 0 | Warning: the coordinates in the 4FGL are consistent with Simbad, but differ of from NED. SDSS offers two sources: a star for the former and a BL Lac for the latter (NVSS ). Both are consistent with the ROSAT source, but the BL Lac is the more reliable source of X- and rays | ||
| J | 7C | 0.398 | Table A2 | bll | BLLAC | 1 | Paggi+ (2014). Marleau+ (2007) suggested a tentative | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | S4 | 0.717 | Stickel+Kühr (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | Steep radio spectrum (), MIS? | ||
| J | PKS | 0.586 | Afanas’ev+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | I Zw 187 | 0.0554 | Oke (1978) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.293 | Peterson+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | MRC | - | - | bcu | UNCL | 3 | Steep radio spectrum (), MIS? | ||
| J | PKS | 1.34 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.166 | Table A2 | bcu | UNCL | 1 | - | ||
| J | GB6 J | 0.204 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.902 | Bolton+ (1981) | fsrq | FSRQ | 0 | - | ||
| J | SDSS J | 0.400 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | B2 A | 0.976 | Stickel+ (1989) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.705 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISEA J | 0.215 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.800 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | MG1 J | 2.39 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.177 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 6C B | - | - | bcu | UNCL | 3 | - | ||
| J | MG2 J | 0.126 | Laurent-Muehleisen+ (1998) | fsrq | SEY | 0 | Laurent-Muehleisen also classified the source as BLRG on the basis of the Ca H+K break, but the radio spectrum is flat. | ||
| J | NVSS J | 0.244 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 1.55 | Stickel+Kühr (1994) | fsrq | FSRQ | 0 | - | ||
| J | S4 | 0.570 | Table A2 | fsrq | BLLAC | 1 | Featureless, Xu+ (1994). A nearby star generated some confusion in early optical observations: see the note in Stickel+Kühr (1993). Later, Stickel+Kühr (1994) reported a preliminary by Xu+ (1994), which was not confirmed in the Xu’s paper. Britzen+ (2008) reported , but its origin is unknown and the value was never confirmed. | ||
| J | 4C | 1.38 | Walsh+ (1979) | fsrq | FSRQ | 0 | LAMOST | ||
| J | 87GB | 0.755 | Table A2 | bll | UNCL | 1 | - | ||
| J | GB6 J | 0.220 | Caccianiga+ (2002) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.610 | Table A2 | bcu | BLLAC | 1 | LAMOST | ||
| J | RGB J | 0.4 | Nilsson+ (2003) | bll | BLLAC | 1 | - | ||
| J | B3 | 1.96 | Falco+ (1998) | fsrq | FSRQ | 0 | - | ||
| J | S3 | 0.084 | Heidt+ (1999) | bll | BLLAC | 0 | Triple interacting system | ||
| J | PKS | 1.05 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.605 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2020) | ||
| J | PMN J | - | - | bll | UNCL | 3 | - | ||
| J | NVSS J | 0.999 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.854 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | B2 C | 0.267 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | Steep radio spectrum, Rector+ (2003) reported an unusual FRI-like strongly-distorted morphology, but core dominated. It acts as gravitational lens for a background galaxy (Heidt+ 1997, Nilsson+ 1999, Lietzen+ 2008). | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.460 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | B3 | 0.785 | Table A2 | bll | BLLAC | 1 | Vermeulen+ (1996). They also found some absorption features and sets , but this lower limit was then taken as an exact value in the subsequent literature | ||
| J | MG2 J | 2.76 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | 87GB | 0.644 | Table A2 | bcu | UNCL | 1 | - | ||
| J | S4 | 0.770 | Arp+ (1976) | bll | BLLAC | 0 | - | ||
| J | B3 | 0.316 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | OT 081 | 0.320 | Stickel+ (1988) | bll | CLAGN | 0 | The in the note by Falomo+ (1993) is clearly a typo | ||
| J | MG2 J | 0.736 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 A | 0.207 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | B2 | 1.12 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.659 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | 1.26 | Shaw+ (2013) | bll | BLLAC | 0 | Tentative, based on the identification of one single line as MgII | ||
| J | MG2 J | 0.544 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 1.48 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.547 | Healey+ (2008) | fsrq | FSRQ | 0 | Early observations were inconclusive, because of featureless spectra. Healey reported the z and classification, but no other information is given, so that it is not possible to understand if there was an intrinsic change of the source or just an improved instrument sensitivity | ||
| J | 87GB | 2.06 | Truebenbach+Darling (2017) | bcu | BLLAC | 0 | Warning: the detected lines fit also well with , but this value is excluded by the non-detection of the host galaxy | ||
| J | MS | 0.407 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | 7C | 0.755 | Shim+ (2013) | bcu | BLLAC | 0 | - | ||
| J | 87GB | 0.152 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | NVSS J | 0.382 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | - | - | bll | BLLAC | 2 | Gioia+ (2003) | ||
| J | S5 | 0.684 | Stickel+ (1993) | bll | CLAGN | 0 | Lawrence+ (1987) took two spectra, the second thirteen months after the first: the first spectrum was quasar-like, while the second one was almost featureless. | ||
| J | 87GB | - | - | bcu | UNCL | 3 | - | ||
| J | S4 | 0.663 | Walsh+Carswell (1982) | fsrq | FSRQ | 0 | Spectrum from Torrealba+ (2012) | ||
| J | PKS | 1.20 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.679 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.960 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 3C 371 | 0.0495 | Sandage (1966) | bll | BLLAC | 0 | Multiple interacting system (Arp 1970, Stickel+ 1993) | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | 7C | 0.239 | Gioia+ (2003) | bll | BLLAC | 0 | Gioia identified the ROSAT source as a cluster of galaxies; no spectrum published, no other information. The radio spectrum is borderline (), but the LAT spectrum is typical of a BLLAC () | ||
| J | RGB J | 0.45 | Nilsson+ (2003) | bll | BLLAC | 1 | - | ||
| J | PMN J | 1.02 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.61 | Landt+ (2001) | fsrq | FSRQ | 0 | - | ||
| J | MG2 J | 0.365 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 0.461 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASX J | 0.142 | Peña-Herazo+ (2019) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.167 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | MG2 J | 0.532 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | 2MASS J | 0.556 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2020) | ||
| J | 87GB | 1.36 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.717 | Table A2 | bll | UNCL | 1 | - | ||
| J | B2 | 0.117 | Giommi+ (1991) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.838 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | 2MASS J | 0.275 | Peña-Herazo+ (2020) | bll | BLLAC | 0 | - | ||
| J | B3 | 1.56 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | B2 | 1.35 | Halpern+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.70 | Titov+ (2017) | fsrq | FSRQ | 0 | - | ||
| J | MG1 J | 0.354 | Shaw+ (2012) | fsrq | NLS1 | 0 | Shaw reported FWHM(H) km/s | ||
| J | MG2 J | 0.715 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | NVSS J | 0.319 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | 7C | 1.69 | Gioia+ (2004) | bcu | FSRQ | 0 | - | ||
| J | OU 134 | 1.13 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 7C | 2.14 | Truebenbach+Darling (2017) | bll | CLAGN | 0 | Shaw+ (2013) reported a featureless spectrum, while Truebenbach+Darling found prominent emission lines | ||
| J | 4C | 0.664 | Lawrence+ (1986) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.253 | Table A2 | bcu | BLLAC | 1 | Stern+Assef (2013). Ackermann+ (2011) proposed , but it was never confirmed in the Shaw’s publications. | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | SUMSS J | 0.9 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | B2 D | - | - | bcu | UNCL | 3 | Steep radio spectrum () | ||
| J | 87GB | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 1.53 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.404 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013 | ||
| J | 3C 380 | 0.690 | Lynds+ (1965) | css | MIS | 0 | Classified as FRII by Zensus+ (2002) | ||
| J | NVSS J | 0.450 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 0.773 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | SUMSS J | - | - | bll | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.216 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | 4C | 0.236 | Table A2 | fsrq | BLLAC | 1 | Schmidt (1974) | ||
| J | PKS | - | - | bll | BLLAC | 2 | Sbarufatti+ (2009) | ||
| J | RX J | 0.427 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | NVSS J | 0.919 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.2 | Table A2 | bll | UNCL | 1 | - | ||
| J | 2MASS J | 0.121 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | GB6 J | 0.3 | Nilsson+ (2003) | bll | BLLAC | 1 | - | ||
| J | AT20G J | 0.454 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.36 | Jauncey+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 87GB | 0.752 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG3 J | 0.288 | Goldoni+ (2021) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.028 | Masetti+ (2013) | bll | BLLAC | 0 | - | ||
| J | S4 | 0.472 | Walsh+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.344 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.421 | Marchesini+ (2019) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.111 | Simpson+ (1993) | rdg | MIS | 0 | 6dF. Classified as FRI by Morganti+ (1993) | ||
| J | TXS | 0.490 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | RX J | 0.870 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | B2 A | 0.798 | Sowards-Emmerd+ (2005) | FSRQ | NLS1 | 0 | Shaw+ (2012) reported FWHM(H) km/s | ||
| J | B2 B | 0.918 | Massaro+ (2015) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.364 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | RGB J | 0.221 | Table A2 | bll | BLLAC | 1 | Laurent-Muehleisen+ (1998) | ||
| J | S4 | 0.657 | Stickel+Kühr (1993) | FSRQ | FSRQ | 0 | - | ||
| J | 1RXS J | 0.243 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG2 J | 0.738 | Table A2 | bll | BLLAC | 1 | Ricci+ (2015) | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | NVSS J | 0.2 | Table A2 | bll | AMB | 1 | Marchesi+ (2018) took an optical spectrum, which resulted to be featureless, and suggested a BLLAC classification. However, Chuprikov+ (2005) classified the source as microquasar candidate | ||
| J | B2 | 0.876 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum, borderline () | ||
| J | S4 | 1.25 | Vermeulen+ (1996) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | 0.212 | Perlman+ (1996) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bll | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | GALEXASC J | 0.471 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.136 | Peña-Herazo+ (2020) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.29 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.076 | de Menezes+ (2020) | fsrq | SEY | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.255 | Healey+ (2008) | fsrq | FSRQ | 0 | Candidate NLS1? Shaw+ (2012) reported FWHM(H) km/s | ||
| J | TXS | 0.476 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | MG2 J | 0.0898 | Paiano+ (2020) | bll | BLLAC | 0 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | Steep radio spectrum () | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | TXS | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.334 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 1.12 | Halpern+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.138 | Marchesini+ (2019) | bll | BLLAC | 0 | - | ||
| J | TXS | 1.10 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.01 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 1.76 | Goncalves+ (1998) | fsrq | FSRQ | 0 | Anguita+ (1979) reported from a personal communication by Bolton, which was never confirmed (spectrum never published). The spectrum published by Goncalves displays two prominent lines identified as CIV and CIII]. Caveat: the Bolton’s value still appears also in the recent literature. | ||
| J | PMN J | 0.6 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.943 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | PMN J | 0.968 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1H | 0.137 | Carangelo+ (2003) | bll | BLLAC | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.196 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | TXS | 0.873 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | WISEA J | 0.430 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Paiano+ (2020) | ||
| J | 1RXS J | 0.4 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.506 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.874 | Halpern+ (2003) | fsrq | FSRQ | 0 | There is a typo in the note on this source, where is reported. However, the published spectrum (Figure 3, bottom right panel) and Table 1 reported the correct value | ||
| J | TXS | 0.6 | Table A2 | bcu | BLLAC | 1 | Desai+ (2019) | ||
| J | PMN J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 0.352 | Wilkes+ (1983) | fsrq | FSRQ | 0 | 6dF | ||
| J | PMN J | 1.28 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.52 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.35 | Table A2 | bll | BLLAC | 1 | Titov+ (2013) | ||
| J | 87GB | 0.112 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | S4 | 0.59 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 0.212 | Peña-Herazo+ (2020) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.518 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.652 | Jauncey+ (1978) | fsrq | FSRQ | 0 | - | ||
| J | GALEXASC J | 1.38 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 1.69 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.445 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | GB6 J | 1.75 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.265 | Landt+ (2001) | bll | BLLAC | 0 | - | ||
| J | 6C B | 1.94 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.965 | Wilkes+ (1983) | fsrq | CLAGN | 0 | The first observation by Peterson+Bolton (1972) resulted in a featureless spectrum. Wilkes+ (1983) reported a tentative value from Jauncey+ in preparation, but the published paper (Jauncey+ 1984) did not contain the source. Nonetheless, the redshift was later confirmed by Stickel+Kühr (1996) and Drinkwater+ (1997). The latter also published the spectrum, where two prominent emission lines – identified as MgII and CIII] – are apparent. The 6dF archive has two low-quality () spectra: the first one, taken on 2022/09/09, displays an emission feature consistent with the MgII line, but it was misidentified with H because of a close artifact; this emission feature is absent in the second spectrum, taken two days later. | ||
| J | PKS | - | - | bcu | UNCL | 3 | Steep radio spectrum () | ||
| J | PKS | 1.66 | Jauncey+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.314 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.588 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) took an extremely noisy spectrum, which makes it impossible to say anything, but background noise. Titov+ (2011) published a low S/N spectrum, with a couple of emission features at Å and Å, which might be CIV and Mg II (then ) | ||
| J | GB6 J | - | - | bcu | UNCL | 3 | - | ||
| J | SUMSS J | 0.2 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.0492 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | SUMSS J | - | - | bcu | BLLAC | 2 | Rajagopal+ (2021) | ||
| J | 1RXS J | 0.247 | Table A2 | bcu | BLLAC | 1 | Rajagopal+ (2021) | ||
| J | AT20G J | 0.6 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.04 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Shaw+ (2013) | ||
| J | CRATES J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 1.08 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | WN B | 0.765 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.2 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.683 | Shaw+ (2012) | bll | BLLAC | 0 | Shaw classified it as FSRQ, but the spectrum is quite noisy and shows only a weak emission line identified as MgII. Titov+ (2013) found a featureless spectrum | ||
| J | 1RXS J | 0.221 | Marchesini+ (2019) | bll | BLLAC | 0 | - | ||
| J | 1RXS | 0.651 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2017) | ||
| J | OV 591 | 1.23 | Strittmatter+ (1974) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 1.00 | Table A2 | bcu | UNCL | 1 | NED has no publication. Simbad has only one star at from the coordinates. | ||
| J | PKS | 1.24 | Jauncey+ (1982) | fsrq | FSRQ | 0 | Peterson+ (1976) identified the source with a radio-quiet (!) galaxy at , but the coordinates are at from the radio position. Wilkes+ (1983) reported no redshift and indicated the Peterson’s object as a close galaxy. Jauncey gave the correct identification and redshift. Please note a typo in the specific note on this source in Jauncey’s paper: it was written PKS instead of PKS | ||
| J | PKS | 0.626 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | - | - | bcu | UNCL | 3 | - | ||
| J | 1RXS J | 0.119 | Mauch+Sadler (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | 2.18 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Ricci+ (2015) | ||
| J | 1ES | 0.0470 | Schachter+ (1993) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.37 | Table A2 | fsrq | UNCL | 1 | The BZCAT by Massaro+ (2009) classified it as FSRQ with , but its origin is unknown. The fifth edition of BZCAT does not contain the source anymore. | ||
| J | TXS | 0.222 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.652 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.417 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.869 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013). The 2FGL catalog (Ackermann+ 2011) reported , referring to the Shaw’s paper yet to be published. However, the published Shaw’s paper reported no redshift measurement | ||
| J | 1RXS J | 0.173 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | - | - | bcu | BLLAC | 2 | Rajagopal+ (2021) | ||
| J | 1RXS J | 0.787 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2016) | ||
| J | 1RXS J | 2.32 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.868 | Hunstead+ (1978) | fsrq | FSRQ | 0 | - | ||
| J | S5 | 0.342 | Stickel+ (1989) | bll | BLLAC | 0 | Gopal-Krishna+Wiita (2000) reported a FRI-FRII hybrid radio morphology. Flat radio spectrum | ||
| J | 87GB | 1.57 | Henstock+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.833 | Wallace+ (2002) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 1.33 | Vermeulen+ (1995) | fsrq | FSRQ | 0 | - | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.240 | Drinkwater+ (1997) | nlsy1 | MIS | 0 | Classified as NLS1 by Oshlack+ (2001). Classified as MIS/CSS by Berton+ (2021) | ||
| J | PKS | 0.0710 | Falomo+ (1987) | BLL | BLLAC | 0 | - | ||
| J | TXS | 0.762 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | 4C | 0.950 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 1.18 | Peterson+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.25 | Table A2 | bll | UNCL | 1 | - | ||
| J | AT20G J | 0.6 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.230 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.341 | Massaro+ (2015) | bll | BLLAC | 0 | - | ||
| J | 4C | 0.243 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.853 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | 0.3 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | S4 | 2.85 | Stickel+Kühr (1993) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bll | BLLAC | 2 | Shaw+ (2013). The 2FGL catalog (Ackermann+ 2011) reported , referring to the Shaw’s paper yet to be published. However, the published Shaw’s paper reported no redshift measurement | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.598 | Hook+ (2003) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.242 | Table A2 | bcu | BLLAC | 1 | Kollatschny+ (2008) | ||
| J | PMN J | 0.473 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016). Massaro+ (2015) proposed the association with NVSS J (FSRQ, ), which is distant from the 4FGL counterpart | ||
| J | 1RXS J | 0.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.085 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | S5 | 0.594 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.625 | Table A2 | bcu | BLLAC | 1 | Titov+ (2013) | ||
| J | PMN J | 0.767 | Table A2 | fsrq | BLLAC | 1 | Shaw+ (2013). The 2FGL catalog (Ackermann+ 2011) reported , referring to the Shaw’s paper yet to be published. However, the published Shaw’s paper reported no redshift measurement | ||
| J | PMN J | 0.164 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 1.03 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | PKS | 1.47 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.624 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.21 | Véron-Cetty+Véron (1993) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.39 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.884 | Shaw+ (2012) | fsrq | CLAGN | 0 | Shaw found prominent emission lines, while Titov+ (2013) published an almost featureless spectrum and classified it as BLLAC (although there is a clear emission line at Å consistent with [OII]). Titov observed in 2011, while Shaw did not publish the dates. | ||
| J | 2MASS J | 0.258 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.760 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.671 | Shaw+ (2012) | fsrq | SEY | 0 | Shaw also classified it as LINER, but the spectrum is quite noisy. To be confirmed with better S/N. Flat radio spectrum | ||
| J | TXS | 0.543 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.610 | Peña-Herazo+ (2017) | fsrq | SEY | 0 | Likely a LINER | ||
| J | PKS | - | - | bcu | UNCL | 3 | - | ||
| J | RX J | 0.668 | Massaro+ (2015) | bll | BLLAC | 0 | - | ||
| J | TXS | 0.687 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.456 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 0.149 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.22 | Stickel+Kühr (1993) | bll | FSRQ | 0 | Stickel+Kühr classified it as BLLAC, but Rector+Stocke (2001) found a strong CIV line at Å ( Å), thus classifying it as FSRQ. The CIV line was not observed in the Stickel+Kühr spectrum, because its blue wavelength threshold was at Å, so it is likely not a CLAGN. | ||
| J | 87GB | 0.791 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.607 | Sowards-Emmerd+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.213 | Table A2 | bll | BLLAC | 1 | Desai+ (2019). However, in the published spectrum there are some weak emission features at and Å, which might be identified with [OII] and [OIII], respectively, at | ||
| J | PKS | 0.601 | Antonucci+ (1987) | fsrq | FSRQ | 0 | Candidate NLS1: Shaw+ (2012) measured FWHM(H) km/s | ||
| J | 87GB | 1.07 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | 1RXS J | 0.237 | Álvarez Crespo+ (2016) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.695 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.569 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 1.98 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.802 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.193 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.57 | Wilkes (1986) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.162 | Guzzo+ (2009) | bll | AMB | 0 | The featureless 6dF spectrum, with just the calcium break, and the gamma-ray photon index quite hard () suggest a BLLAC classification; but the radio spectrum is steep (), suggesting a MIS. | ||
| J | TXS | 1.89 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.3 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | NVSS J | 0.0986 | Guzzo+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | MG2 J | 0.104 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.888 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISEA J | 1.52 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 2MASS J | 0.337 | Table A2 | bll | UNCL | 1 | Peña-Herazo+ (2020) reported a different counterpart (BLLAC, featureless), which is distant | ||
| J | NVSS J | 0.259 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.655 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.440 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | 2MASS J | 0.461 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2020) | ||
| J | PKS | 0.526 | Jones+ (2009) | fsrq | FSRQ | 0 | 6dF | ||
| J | NVSS J | 0.265 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.166 | Table A2 | bll | UNCL | 1 | - | ||
| J | NVSS J | 0.686 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.257 | Piranomonte+ (2007) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.226 | Klindt+ (2017) | bll | BLLAC | 0 | - | ||
| J | CRATES J | 0.331 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.434 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PMN J | 1.63 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.50 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | RX J | - | - | bll | BLLAC | 2 | Piranomonte+ (2007) | ||
| J | RGB J | 0.151 | SDSS | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.440 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS | ||
| J | NVSS J | 0.342 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 1.49 | Jauncey+ (1984) | fsrq | FSRQ | 0 | Additionally, independently measured by Murdoch+ (1984) | ||
| J | SUMSS J | 0.446 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.12 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | - | - | bll | BLLAC | 2 | Titov+ (2011) | ||
| J | PMN J | 1.15 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.0778 | Jones+ (2009) | bcu | BLLAC | 0 | 6dF | ||
| J | MG3 J | 0.650 | Table A2 | bcu | AMB | 1 | There are two tentative spectroscopic values, but no spectrum published, so that it is not possible to understand if one is correct. Falco+ (1998) reported on the basis of an absorption feature identified as Ca H+K break. Muñoz+ (2003) suggested on the basis of some emission features identified as H and H | ||
| J | RX J | 0.204 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.49 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | Wilkes+ (1983) reported a tentative from unpublished data; never confirmed, no spectrum published. | ||
| J | PKS | 0.892 | Table A2 | bcu | BLLAC | 1 | Titov+ (2011) | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.175 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | NVSS J | 0.5 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.38 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | PKS B | 0.672 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.449 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG3 J | 0.644 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.694 | Table A2 | bcu | UNCL | 1 | - | ||
| J | AT20G J | 1.17 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.534 | Table A2 | bcu | BLLAC | 1 | Marchesini+ (2019) | ||
| J | OX 110 | 2.02 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 0.149 | Shaw+ (2013) | bll | BLLAC | 0 | 6dF | ||
| J | PKS | - | - | bll | BLLAC | 2 | Titov+ (2013) | ||
| J | GALEXASC J | 0.276 | Table A2 | bll | BLLAC | 1 | SDSS inconclusive. Perhaps, if the absorption feature at Å is the calcium break and the weak emission feature at Å is MgII | ||
| J | 2MASS J | 0.395 | Table A2 | bcu | UNCL | 1 | - | ||
| Jc | PKS | 2.50 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 1.59 | Shaw+ (2012) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 0.393 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B2 | 0.950 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.211 | Table A2 | agn | UNCL | 1 | - | ||
| J | B2 B | 2.35 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | B2 | 1.51 | Stickel+ (1993) | fsrq | FSRQ | 0 | - | ||
| J | MRSS | 0.285 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.408 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.305 | SDSS | bll | BLLAC | 0 | - | ||
| J | B2 | - | - | bll | BLLAC | 2 | Shaw+ (2013) suggested a tentative on the basis of a very weak emission feature at Å identified as CIV. Paiano+ (2017) found again a featureless spectrum, but cannot confirm Shaw’s weak feature, because her spectrum starts at Å. | ||
| J | 4C | 1.01 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum (), double lobe van Velzen+ (2015), likely a MIS | ||
| J | TXS | 2.3 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.215 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | PMN J | 0.463 | SDSS | fsrq | SEY | 0 | There are some measurements of the FEHM(H) suggesting it might be a NLS1: Shaw+ (2012), km/s; Rakshit+ (2017), km/s; Rakshit+ (2020), km/s. However, the SDSS spectrum shows a broadening of the H profile, indicating a classification as intermediate Seyfert, confirmed by Massaro+ (2014), although with no explanation | ||
| Jc | TXS | 0.260 | SDSS | nlsy1 | SEY | 0 | Classified as NLS1 by Rakshit+ (2017) and Yang+ (2018), it has been reclassified as intermediate Seyfert by Järvelä+ (2020). The radio spectrum is steep at frequencies smaller than GHz, but it becomes flat at higher frequencies (Yang+ 2018). Ongoing merging with a non-jetted Seyfert 2 galaxy (Järvelä+ 2020, Paliya+ 2020) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 1.84 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.582 | Shaw+ (2012) | bcu | SEY | 0 | Shaw classified it as LINER, but it might also be a Seyfert 2 | ||
| J | PMN J | 1.02 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | OX 131 | 2.18 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | OX 036 | 1.94 | Steidel+Sargent (1991) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PMN J | 0.5 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | PKS | 0.612 | Table A2 | FSRQ | UNCL | 1 | Savage+Wright (1981) suggested either or , with a preference for the latter. Jackson+ (2002) found that almost all the redshift estimates of that paper were wrong, and rejected the proposed value. | ||
| J | 87GB | 0.851 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NGC 7059 | - | - | bcu | AMB | 3 | Warning! 4FGL proposed NGC 7059 as counterpart, a starforming SAB galaxy at , but the coordinates in the columns RA_Counterpart and DEC_Counterpart are not consistent with its center (difference ). See the discussion in the Section 3. | ||
| J | B2 | 0.590 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | PMN J | 0.0565 | Jones+ (2009) | bll | BLLAC | 0 | 6dF | ||
| J | SUMSS J | 0.148 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | - | - | bcu | UNCL | 3 | - | ||
| J | RBS 1751 | - | - | bll | BLLAC | 2 | Goldoni+ (2021). 6dF | ||
| J | RBS 1752 | 0.449 | Piranomonte+ (2007) | bll | BLLAC | 0 | Uncertain redshift, but somehow confirmed with caveat by Sbarufatti+ (2009) | ||
| J | RBS 1755 | - | - | bll | BLLAC | 2 | Piranomonte+ (2007) | ||
| J | PMN J | 0.704 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 1.11 | Table A2 | bcu | UNCL | 1 | - | ||
| Jc | 87GB | 0.294 | Massaro+ (2015) | bll | BLLAC | 0 | - | ||
| J | MG1 J | 0.676 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.699 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.285 | Drinkwater+ (1997) | bll | CLAGN | 0 | The first uncertain estimate () was published by Wills+Lynds (1978), but it was not confirmed by subsequent observations. Baldwin+ (1989) reported the detection of two weak narrow emission lines, but they cannot identify them. Stickel+ (1993) and Verón-Cetty+Verón (1993) reported featureless spectra. Drinkwater+ (1997) confirmed the lines detected by Baldwin+ (1989), with the addition of one more, which was identified as CIV and allowed to measure . This result was definitely confirmed by Rector+Stocke (2001), who also reported equivalent width stronger than 5 Å, thus suggesting a CLAGN classification. The automatic pipeline of SDSS failed to find the redshift, likely because of the strong artifact at Å: [OII] is misidentified as H, MgII as H, and it missed the evident line at Å (which is CIII]). | ||
| J | PKS | 0.632 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.501 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | PMN J | 2.18 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | OX 057 | 1.94 | Shimmins+ (1968) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.941 | SDSS | bcu | FSRQ | 0 | - | ||
| J | MG3 J | 0.629 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.290 | Piranomonte+ (2007) | bll | BLLAC | 0 | - | ||
| J | PMN J | 1.44 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MH | 0.468 | Table A2 | bll | BLLAC | 1 | Landoni+ (2014). Monroe+ (2016) reported , but the published spectrum does not show any evident feature supporting that claim | ||
| J | B2 | 1.31 | Britzen+ (2007) | bcu | UNCL | 0 | Britzen reported the redshift from a personal communication by R. Vermeulen, but no classification is given. Henstock+ (1997) observed it with 300 s exposure at the Isaac Newton Telescope, but reported no detection. No other observation is available. | ||
| J | PMN J | 2.01 | Shaw+ (2012) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.959 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | PKS | 0.423 | Brinkmann+ (1994) | fsrq | FSRQ | 0 | 6dF | ||
| J | 2MASS J | 0.156 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.37 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.344 | Wills+Wills (1976) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.760 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CTS 0561 | 1.92 | Maza+ (1995) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.429 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | OX 169 | 0.211 | Wills+Wills (1974) | fsrq | FSRQ | 0 | Extended optical structures due to a recent merger (Hutchings+Neff 1992; McLure+ 1999), double-peaked H (Marziani+ 1996) | ||
| J | MG3 J | - | - | bcu | UNCL | 3 | - | ||
| J | MG3 J | 0.623 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | PKS | 0.334 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.159 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.36 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | 87GB | 0.499 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | MS | 0.237 | Stocke+ (1991) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.698 | Peterson+ (1976) | fsrq | FSRQ | 0 | Oshlack+ (2002) reported FWHM(H) km/s on the basis of the spectrum taken by Drinkwater+ (1997). However, the published spectrum does not seem to match the proposed measurement: it displays evident H (with a broadening toward the continuum) and [OIII], and a rather weak/almost absent [OIII]. The comparison of H with the nearby [OIII] clearly shows the different profiles. Moreover, such a narrow H would point to an obscured object (Seyfert 2?), but the radio spectrum is flat. Jackson+Browne (1991a, 1991b) obtained a better spectrum for the H-[OIII] complex and measured FWHM(H) ∼ 76–66 Å (rest frame), corresponding to a very broad component, typical of FSRQs. | ||
| J | NVSS J | 0.481 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | MG1 J | 1.18 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.11 | White+ (1988) | FSRQ | FSRQ | 0 | Wills+Wills (1976) suggested a tentative never confirmed | ||
| J | PKS | 1.14 | Jauncey+ (1978) | FSRQ | FSRQ | 0 | - | ||
| J | SDSS J | 0.332 | SDSS | bll | AMB | 0 | The SDSS spectrum is quite noisy with a strong gap in the range ∼ 8000–8400 Å. The complex around Å (quite noisy) has been identified with H-[NII], but if it is H-[OIII], then | ||
| J | PKS | 0.999 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | Kinman+Burbidge (1967) suggested a tentative , challenged by Oke+ (1970), who in turn suggested . LAMOST | ||
| J | PKS | 0.203 | Drinkwater+ (2010) | bcu | SEY | 0 | SDSS | ||
| J | PKS B | 0.363 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | TXS | 1.35 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.229 | Fischer+ (1998) | bll | BLLAC | 0 | - | ||
| J | MRSS | 0.186 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.865 | Croom+ (2001) | fsrq | FSRQ | 0 | 6dF | ||
| J | NVSS J | 0.326 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 1.48 | Croom+ (2004) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 2.35 | Wilkes+ (1983) | fsrq | FSRQ | 0 | Wilkes cites a paper by Jauncey in preparation, but no publication was found. The redshift was later confirmed by Wilkes (1986) and many other authors | ||
| J | RBS 1791 | 0.641 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | S3 | 0.874 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | RBS 1792 | 0.342 | SDSS | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.703 | Table A2 | fsrq | UNCL | 1 | Massaro+ (2009) gives FSRQ classification and of unknown origin. | ||
| J | RX J | 1.36 | Table A2 | bll | BLLAC | 1 | Álvarez Crespo+ (2016) | ||
| J | PKS | 0.0283 | Marenbach+Appenzeller (1982) | rdg | MIS | 0 | Classified as FRI by Morganti+ (1993). Optical spectrum type Seyfert 1/LINER, SA0 host galaxy. | ||
| J | PKS B | 0.495 | Hook+ (2003) | fsrq | BLLAC | 0 | - | ||
| J | NVSS J | 0.577 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | B2 | 1.49 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.672 | White+ (1988) | fsrq | CLAGN | 0 | Peterson+ (1978) observed a featureless spectrum, while White’s spectrum has several prominent emission lines. | ||
| J | PKS | 0.116 | Falomo+ (1993) | bll | BLLAC | 0 | - | ||
| J | LEDA 3218689 | 0.271 | Colless+ (2001) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.581 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.470 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | TXS | 0.172 | Afanas’ev+ (2006) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.62 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.121 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.149 | de Menezes+ (2020) | bcu | BLLAC | 0 | - | ||
| J | PKS | 1.87 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | RBS 1813 | 0.169 | Bauer+ (2000) | bll | BLLAC | 0 | Note that Schwope+ (2000) reported and flagged it as uncertain | ||
| J | BL Lac | 0.0686 | Oke+Gunn (1974) | BLL | BLLAC | 0 | - | ||
| J | MS | 0.0489 | Stocke+ (1991) | bll | MIS | 0 | Classified as FR0 by Glowaki+ (2017) | ||
| J | PKS | 1.08 | Smith+ (1977) | fsrq | FSRQ | 0 | - | ||
| J | 4C | 0.0270 | Wills+Wills (1976) | bll | SEY | 0 | Although it is classified as BL Lac Object, Verón-Cetty+Verón (1993) clearly showed a Seyfert-1 type nucleus literally flooded by the host galaxy emission, given the small distance (SDSS image of the host). Scarpa+ (1999) showed the presence of an optical jet. | ||
| J | MG3 J | 0.0730 | Marchã+ (1996) | bll | BLLAC | 0 | - | ||
| J | S5 | 1.38 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 1.05 | Shaw+ (2013) | bll | BLLAC | 0 | SDSS spectrum is noisy, so that the automatic pipeline failed to identify the MgII line at Å | ||
| J | 1RXS J | - | - | bcu | UNCL | 3 | - | ||
| J | 87GB | 1.64 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.21 | Wilkes+ (1983) | fsrq | FSRQ | 0 | Browne+ (1975) reported , but it was challenged by Wilkes. | ||
| J | PMN J | 0.970 | Peña-Herazo+ (2021) | bcu | CLAGN | 0 | SDSS spectrum is featureless, while LAMOST displays a broad emission line identified as MgII. | ||
| J | PMN J | 0.524 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.618 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum () | ||
| J | NVSS J | 0.397 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.900 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.220 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RX J | 0.362 | SDSS | bll | BLLAC | 0 | - | ||
| J | PKS | 0.392 | Peterson+ (1976) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.2 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 1.13 | Sowards-Emmerd+ (2003) | fsrq | CLAGN | 0 | Hook+ (1996) reported a featureless spectrum, although the published image shows a weak feature at Å consistent with MgII. SDSS spectrum displays a prominent MgII line, which could have not been missed by Hook, if present at that epoch | ||
| J | PMN J | 0.280 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG3 J | 0.499 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019). SDSS inconclusive, although there is one weak emission feature at Å, which might be MgII at | ||
| J | TXS | 1.12 | Amirkhanyan+ (2004) | fsrq | FSRQ | 0 | LAMOST | ||
| J | PKS | 1.83 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | SUMSS J | 0.378 | Table A2 | bll | BLLAC | 1 | Marchesini+ (2019) | ||
| J | S3 | 2.46 | Healey+ (2008) | fsrq | FSRQ | 0 | - | ||
| J | B2 B | 0.505 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | SDSS reported , by identifying the emission line at Å as MgII. Since the shape of the continuum is typical of a BLLAC, the cited line is more likely [OII] at . The value has been also confirmed by another spectrum taken by Healey+ (2008). Shaw+ (2013) reported a featureless spectrum, likely due to an increased jet activity | ||
| J | GALEXASC J | 0.690 | Table A2 | bcu | UNCL | 1 | - | ||
| J | MG1 J | 1.07 | Shaw+ (2012) | fsrq | FSRQ | 0 | Sowards-Emmerd+ (2005) reported , but it was flagged as uncertain | ||
| J | PKS | 0.901 | Lynds (1967) | fsrq | FSRQ | 0 | - | ||
| J | RX J | 0.149 | SDSS | bll | BLLAC | 0 | Marchesi+ (2018) reported a featureless spectrum, likely due to an increase of the jet activity | ||
| J | PMN J | 0.748 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | NVSS J | - | - | fsrq | UNCL | 3 | - | ||
| J | TXS | 1.39 | Afanas’ev+ (2006) | bcu | FSRQ | 0 | - | ||
| J | SDSS J | 0.616 | Table A2 | bll | BLLAC | 1 | Featureless, Shaw+ (2013). Massaro+ (2014) suggested a tentative on the basis of the SDSS spectrum. There are two weak emission features at Å and Å, which might be identified as [OIII] | ||
| J | PKS | 0.115 | Hook+ (2003) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.1 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.293 | SDSS | bcu | SEY | 0 | Sy2/LINER? | ||
| J | PKS | 0.997 | Sbarufatti+ (2006) | bll | BLLAC | 0 | - | ||
| J | PKS | 1.96 | Arp (1970) | fsrq | FSRQ | 0 | SDSS | ||
| J | 3C 446 | 1.40 | Schmidt (1966) | fsrq | CLAGN | 0 | Many authors reported significant optical spectral variability (e.g., Stephens+Miller 1984, Barbieri+ 1985, Perez+ 1989, …) | ||
| J | 2MASS J | 0.450 | SDSS | bcu | BLLAC | 0 | - | ||
| J | PKS B | 2.26 | Hook+ (2003) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.503 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PKS | 0.0581 | Stein (1996) | rdg | MIS | 0 | Classified FRI by Angioni (2020) | ||
| J | RBS 1864 | - | - | bcu | BLLAC | 2 | 6dF inconclusive, although there is an emission-line complex at Å: if identified as H-[OIII], then . Schwope+ (2000) suggested a tentative and a classification as X-ray Transient Galaxy (XTG). | ||
| J | 2MASS J | 0.525 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.440 | Paiano+ (2019) | bll | BLLAC | 0 | The optical counterpart SDSS J is distant from the radio centroid, although still consistent with the position error of NVSS (). | ||
| J | PKS | 0.907 | Titov+ (2017) | bcu | FSRQ | 0 | - | ||
| J | PKS | 1.56 | Wilkes+ (1983) | FSRQ | FSRQ | 0 | SDSS | ||
| J | PKS | 0.511 | Peña-Herazo+ (2021) | bcu | FSRQ | 0 | - | ||
| J | PKS | 1.33 | White+ (1988) | fsrq | FSRQ | 0 | - | ||
| J | CTA 102 | 1.04 | Schmidt (1965) | FSRQ | FSRQ | 0 | - | ||
| J | NVSS J | 0.386 | Jiménez-Bailón+ (2012) | bll | BLLAC | 0 | - | ||
| J | RX J | 0.214 | Caccianiga+ (2002) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.181 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PMN J | 0.252 | Table A2 | bll | UNCL | 1 | - | ||
| J | PMN J | 0.520 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.506 | Jauncey+ (1984) | fsrq | FSRQ | 0 | 6dF | ||
| J | NVSS J | 0.442 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | PKS | 0.647 | Hook+ (2003) | bll | BLLAC | 0 | - | ||
| J | B2 A | 0.795 | Schmidt (1977) | fsrq | CLAGN | 0 | Richstone+Schmidt (1980) reported EW(MgII) Å, while Shaw+ (2013) found a weak MgII line and classified the source as BLLAC. The prominent MgII is also clearly visible in the optical spectrum published by Jackson+Browne (1991) | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 1.52 | Table A2 | BLL | BLLAC | 1 | Shaw+ (2013). Warning: in the literature, it is often reported , with reference to Johnston+ (1995), who in turn referred to Schmidt+Green (1983), but the latter paper does not contain the source. The featureless spectrum has been reported by other authors, and Shaw is just the latest one. | ||
| J | NVSS J | 0.235 | de Menezes+ (2020) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.297 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.569 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | 1RXS J | 0.167 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.134 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISEA J | 1.15 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.726 | Britzen+ (2007) | bll | BLLAC | 0 | Meisner+Romani (2010) estimated an imaging , which is sometimes adopted in the literature. The Britzen’s value is spectroscopic, based on the detection of two oxygen lines and the calcium break | ||
| J | 1RXS J | 0.553 | SDSS | bcu | BLLAC | 0 | - | ||
| J | PKS | 0.774 | Stickel+ (1993) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 1.20 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RBS 1888 | 0.226 | Fischer+ (1998) | bll | BLLAC | 1 | - | ||
| J | PMN J | 1.62 | Table A2 | bcu | UNCL | 1 | - | ||
| J | RGB J | 0.53 | Rosa González+ (2019) | bll | BLLAC | 1 | - | ||
| J | TXS | 1.17 | Shaw+ (2012) | fsrq | FSRQ | 0 | - | ||
| J | NVSS J | 0.641 | Sandrinelli+ (2013) | bll | BLLAC | 0 | SDSS inconclusive | ||
| J | NVSS J | 0.653 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.597 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | RBS 1895 | 0.194 | Beuermann+ (1999) | bcu | BLLAC | 0 | - | ||
| J | PKS | 0.949 | Shaw+ (2013) | bll | BLLAC | 0 | There are many spectra with different results. Hook+ (2003) suggested a tentative on the basis of the identification of a line at Å as OII. Sandrinelli+ (2013) found a featureless spectrum, but her wavelength interval starts at Å. Shaw+ (2013) suggested on the basis of two lines, one at Å identified as MgII, and the other at Å should be [OII]; no line at Å. The SDSS spectrum is quite noisy, but it confirms the line at Å, which implies that the line detected by Hook might be CIII]. | ||
| J | PKS | 2.25 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | RGB J | 1.90 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | PKS | 2.27 | Peterson+ (1979) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.28 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS. Hook+ (1996) reported a featureless spectrum, although a weak line at Å corresponding to MgII is visible | ||
| J | RBS 1899 | 0.607 | Sbarufatti+ (2009) | bll | BLLAC | 0 | Landoni+ (2013) cast some doubts, because the features seems to be contaminated by atmospheric absorption | ||
| J | SUMSS J | 0.241 | Table A2 | bcu | UNCL | 1 | - | ||
| J | WISEA J | 0.763 | Table A2 | bcu | UNCL | 1 | - | ||
| J | B3 | 0.119 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | LAMOST | ||
| J | PKS | 0.599 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 0.344 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.289 | Table A2 | bll | UNCL | 1 | Hewitt+Burbidge (1993) reported from the PhD thesis of M. Drinkwater (1987). Ackermann+ (2011) reported of unknown origin. | ||
| J | PMN J | 0.525 | Shaw+ (2012) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.142 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 0.246 | Böhringer+ (2004) | bcu | BLLAC | 0 | - | ||
| J | MG4 J | 0.229 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | 2MASS J | 0.497 | SDSS | bll | BLLAC | 0 | - | ||
| J | TXS | 0.822 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum () | ||
| J | CRATES J | 0.258 | Pursimo+ (2013) | bcu | FSRQ | 0 | Optical spectrum published in Titov+ (2017) | ||
| J | NVSS J | 0.327 | SDSS | bll | BLLAC | 0 | - | ||
| J | 3C | 0.858 | Lynds (1967) | FSRQ | FSRQ | 0 | LAMOST | ||
| J | B3 | 0.105 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.333 | Londish+ (2002) | bll | BLLAC | 0 | - | ||
| J | MG3 J | 0.547 | Table A2 | bll | BLLAC | 1 | Paiano+ (2019). Possible neutrino source. SDSS inconclusive, although two weak emission features might point to : Å CIII], Å MgII | ||
| J | PKS | 1.75 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | - | - | bcu | UNCL | 3 | - | ||
| J | PKS | 0.858 | Table A2 | bll | BLLAC | 1 | Landoni+ (2014) | ||
| J | NVSS J | 0.513 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | OY 91 | 0.191 | Stickel+ (1988) | bll | BLLAC | 0 | LAMOST | ||
| J | PKS | 0.926 | Browne+ (1975) | fsrq | FSRQ | 0 | 6dF | ||
| J | MRSS | 0.319 | Table A2 | bll | BLLAC | 1 | Landoni+ (2015) | ||
| J | PMN J | 0.479 | Landt+ (2004) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.252 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | - | - | fsrq | UNCL | 3 | - | ||
| J | GALEXASC J | 1.62 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.238 | Table A2 | bll | BLLAC | 1 | Marchesi+ (2018) | ||
| J | NVSS J | 0.502 | Table A2 | bll | BLLAC | 1 | Titov+ (2017) | ||
| J | PKS | 1.48 | Wilkes+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | 87GB | 1.75 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS B | 0.777 | Hook+ (2003) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.129 | Searle+Bolton (1968) | rdg | MIS | 0 | Classified as FRI by Heckman+ (1984). Tidal interaction with close companion, precessing jet, Hunstead+ (1984). 6dF | ||
| J | PKS | 1.27 | White+ (1988) | bcu | FSRQ | - | LAMOST spectrum found the correct redshift, but it displays also an unknown strong emission line at Å: artifact? | ||
| J | 1RXS J | - | - | bll | BLLAC | 2 | Shaw+ (2013). Wu+ (2012) reported of unknown origin. | ||
| J | RBS 1943 | 0.640 | Table A2 | bll | UNCL | 1 | - | ||
| J | 1RXS J | 0.681 | Table A2 | bll | BLLAC | 1 | Piranomonte+ (2007). | ||
| J | MG1 J | 0.503 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | Sowards-Emmerd classified the source as Narrow-Line Radio Galaxy (spectrum not shown, no information on emission lines). Newer observations by Healey+ (2008), Shaw+ (2013), and SDSS showed only a featureless spectrum, thus suggesting a BLLAC classification, favored also by the inverted radio spectrum (). | ||
| J | MG1 J | 0.824 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum () | ||
| J | WISEA J | - | - | bcu | BLLAC | 2 | Rajagopal+ (2021) | ||
| J | NVSS J | 0.497 | Table A2 | bll | BLLAC | 1 | Titov+ (2017). SDSS and LAMOST inconclusive (although the latter shows some absorption features, which might be the calcium break and the G band at | ||
| J | B2 | 1.82 | Wills+Wills (1976) | FSRQ | FSRQ | 0 | SDSS | ||
| J | MG3 J | 1.75 | SDSS | bcu | FSRQ | 0 | - | ||
| J | MG4 J | 1.45 | Vermeulen+Taylor (1995) | fsrq | FSRQ | 0 | - | ||
| J | CRATES J | 2.02 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.5 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 87GB | 1.19 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 2.88 | Stickel+ (1989) | bcu | FSRQ | 0 | - | ||
| J | RGB J | 0.164 | Sowards-Emmerd+ (2005) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 0.811 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | SUMSS J | 0.646 | Marchesini+ (2019) | bll | BLLAC | 0 | - | ||
| J | B3 | 1.10 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SUMSS J | 0.150 | Table A2 | bll | BLLAC | 1 | 6dF | ||
| J | TXS | 2.16 | SDSS | bcu | FSRQ | 0 | - | ||
| J | PKS | 0.0543 | Crawford+Fabian (1994) | bll | BLLAC | 0 | 6dF. Gioia+Luppino (1994) reported : typo? | ||
| J | RX J | 0.152 | Table A2 | bll | BLLAC | 1 | Landoni+ (2013) | ||
| J | PKS | 3.16 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | 2MASS J | 0.200 | Schwope+ (2000) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.694 | Paiano+ (2019) | bll | BLLAC | 0 | - | ||
| J | PMN J | 0.17 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | 4C | 1.26 | Stickel+Kühr (1992) | fsrq | FSRQ | 0 | SDSS. Sargent (1973) associated this source with the cluster A2584 (), but it is behind it, as proved by Stickel+Kühr. | ||
| J | B2 | 1.49 | Shaw+ (2012) | fsrq | FSRQ | 0 | Marchã+ (1996) reported a featureless spectrum, but due to low source flux (∼ erg cm s Å to be compared with Shaw’s value erg cm s Å), which resulted in a low S/N spectrum. However, a weak CIII] line can be spotted | ||
| J | B3 | 1.25 | Britzen+ (2008) | fsrq | BLLAC | 0 | Sowards-Emmerd+ (2005) reported flagged as uncertain and a FSRQ classification. However, other published spectra are featureless (Hook+ 1996, Henstock+ 1997) or with weak features (Truebenbach+Darling 2017, perhaps an [OIII] line in Sp1) | ||
| J | PMN J | 0.686 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.0964 | Laurent-Muehleisen+ (1998) | bll | BLLAC | 0 | LAMOST | ||
| J | SUMSS J | 0.372 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013) | ||
| J | PKS | 1.41 | Browne+ (1975) | fsrq | FSRQ | 0 | - | ||
| J | TXS | 2.14 | Titov+ (2011) | fsrq | FSRQ | 0 | - | ||
| J | 1ES | - | - | bll | BLLAC | 2 | Paiano+ (2017). Perlman+ (1996) proposed , but this value was never confirmed, despite of the several attempts, and has been definitely confuted by Paiano. There is also an inconclusive LAMOST spectrum. | ||
| J | PMN J | 0.65 | Table A2 | bll | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | 1ES | 0.174 | Goldoni+ (2021) | bll | BLLAC | 0 | - | ||
| J | B3 | 0.936 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013) | ||
| J | CTS 0490 | 0.360 | Maza+ (1995) | fsrq | AMB | 0 | Maza published the redshift value only, no spectrum, no information about the emission lines. No other spectra or line information have been published. | ||
| J | PKS | 0.221 | Hook+ (2003) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.355 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | MG1 J | 0.413 | Table A2 | bcu | UNCL | 1 | - | ||
| J | SDSS J | 1.60 | SDSS | bcu | FSRQ | 0 | - | ||
| J | PKS | 0.189 | Stickel+ (1993) | rdg | MIS | 0 | SDSS. Classified FRII by Angioni (2020) | ||
| J | NVSS J | 0.254 | Table A2 | bcu | UNCL | 1 | Peña-Herazo+ (2021) classified it as BLLAC on the basis of LAMOST DR5 data, but the spectrum is no more available in DR7 | ||
| J | PKS | 1.85 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 1.97 | Titov+ (2013) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.946 | Landt+ (2001) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 1.36 | Table A2 | bll | BLLAC | 1 | Masetti+ (2013). Ackermann+ (2011) reported , but the value was not confirmed by Shaw+ (2013) | ||
| J | PKS | 1.30 | Peterson+Bolton (1972) | fsrq | FSRQ | 0 | 6dF | ||
| J | PKS | 0.518 | Jauncey+ (1984) | FSRQ | FSRQ | 0 | - | ||
| J | PKS | 0.0308 | Jones+ (2009) | rdg | MIS | 0 | 6dF. Classified FRI by Angioni (2020) | ||
| J | 2MASS J | 1.19 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 4C | 1.50 | Smith+ (1977) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.279 | Landt+ (2001) | bll | BLLAC | 0 | 6dF | ||
| J | PMN J | 0.563 | Halpern+Crotts (2009) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 1.28 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.15 | Wright+ (1983) | fsrq | FSRQ | 0 | - | ||
| J | GALEXASC J | 0.560 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.671 | Drinkwater+ (1997) | fsrq | FSRQ | 0 | - | ||
| J | PKS B | 1.06 | Perlman+ (1998) | fsrq | FSRQ | 0 | SDSS | ||
| J | TXS | 0.401 | Sowards-Emmerd+ (2005) | fsrq | FSRQ | 0 | SDSS | ||
| J | NVSS J | 0.877 | Table A2 | bll | BLLAC | 1 | Shaw+ (2013). | ||
| J | PKS | 0.0477 | Wills+Wills (1976) | agn | CLAGN | 0 | The jet changed its viewing angle, from a MIS to a SEY, Hernández-García+ (2017) | ||
| J | PKS | 1.19 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | SDSS | ||
| J | PMN J | 0.147 | Table A2 | bll | UNCL | 1 | - | ||
| J | B2 | 0.127 | Owen+ (1995) | bcu | MIS | 0 | Classified FRI in the same paper | ||
| J | PKS | 1.41 | Hook+ (2003) | fsrq | FSRQ | 0 | - | ||
| J | PMN J | 0.672 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 1.07 | Wills+Lynds (1978) | fsrq | FSRQ | 0 | SDSS | ||
| J | PKS | 0.269 | Verón-Cetty+Verón (1993) | agn | CLAGN | 0 | Early observations by Strittmatter+ (1974) reported a continuous spectrum. Additionally, Wills+Lynds (1978) found the same, with the exception of a feature at Å, which they judge unreliable. For some time, this source was classified as BLLAC, until Verón-Cetty+Verón reported a Seyfert 2-type spectrum, and identified the Wills+Lynds’ feature as [OII]. SDSS spectrum confirms. | ||
| J | RX J | 0.291 | Owen+ (1995) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.139 | Table A2 | bll | BLLAC | 1 | Desai+ (2019) | ||
| J | NVSS J | 1.41 | Table A2 | bcu | UNCL | 1 | - | ||
| J | CRATES J | 2.66 | Pursimo+ (2013) | bcu | FSRQ | 0 | SDSS | ||
| J | GALEXASC J | 0.293 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1RXS J | 0.274 | Caccianiga+ (2002) | bll | BLLAC | 0 | - | ||
| J | PKS | 0.0523 | Rhee+Katgert (1992) | rdg | MIS | 0 | Classified FR0 by Glowacki+ (2017) | ||
| J | 1RXS J | 0.365 | Piranomonte+ (2007) | bll | BLLAC | 0 | SDSS | ||
| J | PKS | 1.24 | Pierre+ (2016) | bcu | MIS | 0 | Steep radio spectrum (), classified as HERG by Chiappetti+ (2018). | ||
| J | 1RXS J | 0.131 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | PMN J | 0.621 | Healey+ (2008) | FSRQ | CLAGN | 0 | Changing SED, Ghisellini+ (2013) | ||
| J | TXS | 0.172 | Paiano+ (2017) | bll | BLLAC | 0 | SDSS | ||
| J | WN B | - | - | bll | BLLAC | 2 | Healey+ (2008) | ||
| J | PKS | 0.576 | Murdoch+ (1984) | fsrq | FSRQ | 0 | Borderline FSRQ/NLS1, FWHM(H) Å km/s (see also Jackson+Browne 1991) | ||
| J | PKS | 0.184 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.707 | Table A2 | bcu | UNCL | 1 | - | ||
| J | TXS | 0.819 | Table A2 | bcu | BLLAC | 1 | Peña-Herazo+ (2021) | ||
| J | TXS | 0.419 | Sbarufatti+ (2009) | fsrq | CLAGN | 0 | The same paper describes the change in the optical spectrum | ||
| J | LEDA 3231681 | 0.233 | Colless+ (2001) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.127 | Table A2 | bcu | BLLAC | 1 | 6dF | ||
| J | SUMSS J | 0.245 | Table A2 | bll | UNCL | 1 | - | ||
| J | CLASS J | 0.448 | Table A2 | bll | BLLAC | 1 | Massaro+ (2015) | ||
| J | MG3 J | 0.876 | SDSS | bcu | FSRQ | 0 | - | ||
| J | 2MASS J | 0.250 | Table A2 | bcu | UNCL | 1 | - | ||
| J | 1REX J | 0.623 | Table A2 | bll | UNCL | 1 | - | ||
| J | PKS | 0.737 | Shaw+ (2013) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.446 | Table A2 | bcu | UNCL | 1 | - | ||
| J | NVSS J | 0.722 | Table A2 | bll | BLLAC | 1 | SDSS | ||
| J | PMN J | 0.272 | Drinkwater+ (2018) | fsrq | AMB | 0 | Neither the spectrum, nor a classification was published. The redshift is based on the detection of one line identified as [OII], which suggests a BLLAC identification, although the LAT spectrum is rather soft. Massaro+ (2015) classified it as FSRQ with , but no other information is given. | ||
| J | 4C | 1.99 | Stickel+Kühr (1993) | fsrq | FSRQ | 0 | The featureless object observed by Peterson+ (1978) is distant from the radio position | ||
| J | S5 | 1.34 | Vermeulen+ (1996) | fsrq | FSRQ | 0 | The early classification as featureless BL Lac object made by Stickel+Kühr (1993) was due to a low S/N spectrum. The emission features in Vermeulen’s spectrum are visible also in the Stickel+Kühr’s one. | ||
| J | NVSS J | 0.9 | Table A2 | bcu | UNCL | 1 | Steep radio spectrum (), classified as radiogalaxy by Zanichelli+ (2001) | ||
| J | NVSS J | 0.0937 | Table A2 | bll | BLLAC | 1 | Two values of redshift were proposed, but none is convincing. Ackermann+ (2011) reported (spectrum not shown), while Massaro+ (2015) measured on the basis of an almost featureless spectrum. LAMOST inconclusive | ||
| J | PKS | 0.554 | Table A2 | bcu | UNCL | 1 | - | ||
| J | PKS | 0.812 | Sbarufatti+ (2005) | bll | BLLAC | 0 | - | ||
| J | RBS 2066 | 2.33 | Table A2 | bll | BLLAC | 1 | Sbarufatti+ (2009) | ||
| J | PKS | 1.01 | Jauncey+ (1984) | fsrq | FSRQ | 0 | - | ||
| J | PKS | 0.444 | Healey+ (2008) | bcu | FSRQ | 0 | - | ||
| J | PMN J | 0.891 | Table A2 | bcu | UNCL | 1 | Classified as radiogalaxy by Zanichelli+ (2001) | ||
| J | B3 | 0.200 | Marchesi+ (2018) | bll | SEY | 0 | The better spectrum by Paiano+ (2019) displays several narrow emission lines, typical of Seyfert 2 galaxies. Flat radio spectrum | ||
| J | PKS | 1.64 | Wilkes+ (1983) | fsrq | FSRQ | 0 | SDSS | ||
| J | 1RXS J | 1.17 | Table A2 | bll | BLLAC | 1 | Paiano+ (2019). | ||
| J | B2 | 1.20 | Vermeulen+ (1995) | fsrq | FSRQ | 0 | - | ||
| J | H | 0.165 | Falomo (1991) | bll | BLLAC | 0 | - | ||
| J | 1RXS J | 0.877 | Table A2 | bcu | BLLAC | 1 | SDSS | ||
| J | TXS | 0.0960 | McCarthy+ (1996) | bll | BLLAC | 0 | - | ||
| J | NVSS J | 0.257 | Table A2 | bcu | UNCL | 1 | Classified as radiogalaxy by Zanichelli+ (2001) |
Table A2.
This table reports the photometric redshifts calculated as unweighted arithmetic mean of the number N of photo-redshifts collected from the literature. is the population standard deviation calculated according to for . If , then . If , then is undefined. The references are indicated in the last column and are: (1) DiPompeo+ (2015); (2) Yang+Shen (2022); (3) Kunsági-Máté+ (2022); (4) Flesch (2021); (5) Bilicki+ (2014); (6) Bilicki+ (2016); (7) Ahumada+ (2020); (8) Brescia+ (2014); (9) Gao+ (2018); (10) Lopes (2007); (11) Beck+ (2021); (12) Zou+ (2022), with 12a = DES DR2; 12b = DESI DR9; 12c = HSC SSP PDR3; (13) Zhou+ (2022)—from NOIRlab. The first four columns reported the 4FGL name, right ascension and declination of the optical counterpart (see Section 3 in case of discrepancies with Table A1), and the revised classification as from Table A1.
Table A2.
This table reports the photometric redshifts calculated as unweighted arithmetic mean of the number N of photo-redshifts collected from the literature. is the population standard deviation calculated according to for . If , then . If , then is undefined. The references are indicated in the last column and are: (1) DiPompeo+ (2015); (2) Yang+Shen (2022); (3) Kunsági-Máté+ (2022); (4) Flesch (2021); (5) Bilicki+ (2014); (6) Bilicki+ (2016); (7) Ahumada+ (2020); (8) Brescia+ (2014); (9) Gao+ (2018); (10) Lopes (2007); (11) Beck+ (2021); (12) Zou+ (2022), with 12a = DES DR2; 12b = DESI DR9; 12c = HSC SSP PDR3; (13) Zhou+ (2022)—from NOIRlab. The first four columns reported the 4FGL name, right ascension and declination of the optical counterpart (see Section 3 in case of discrepancies with Table A1), and the revised classification as from Table A1.
| 4FGL Name | RA | DEC | R-Class | N | References | ||
|---|---|---|---|---|---|---|---|
| J0001.2+4741 | 0.3293 | 47.7002 | UNCL | 0.545 | 0.005 | 2 | 3,6 |
| J0001.2−0747 | 0.3251 | −7.7741 | BLLAC | 0.382 | 0.335 | 2 | 3,13 |
| J0001.5+2113 | 0.3849 | 21.2267 | NLS1 | 0.380 | 0.351 | 4 | 1,3,12b,13 |
| J0001.6−4156 | 0.3865 | −41.9237 | UNCL | 0.290 | 0.223 | 3 | 2,12a,13 |
| J0002.1−6728 | 0.5633 | −67.4482 | BLLAC | 0.220 | - | 1 | 6 |
| J0002.3−0815 | 0.6503 | −8.2590 | UNCL | 0.545 | 0.244 | 4 | 1,3,4,13 |
| J0002.4−5156 | 0.6217 | −51.8743 | UNCL | 0.717 | 0.471 | 4 | 2,4,6,13 |
| J0003.1−5248 | 0.8317 | −52.7909 | UNCL | 0.309 | 0.136 | 4 | 2,4,12a,13 |
| J0003.3−1928 | 0.8278 | −19.4562 | UNCL | 0.711 | 0.216 | 3 | 1,3,4 |
| J0003.3−5905 | 0.8055 | −59.0966 | UNCL | 0.636 | 0.218 | 2 | 2,13 |
| J0003.9−1149 | 1.0205 | −11.8162 | BLLAC | 0.519 | 0.280 | 2 | 3,13 |
| J0004.0+0840 | 0.9968 | 8.6939 | BLLAC | 1.362 | 0.693 | 3 | 1,3,13 |
| J0004.3+4614 | 1.0672 | 46.2550 | FSRQ | 1.622 | - | 1 | 3 |
| J0004.4−4737 | 1.1486 | −47.6054 | FSRQ | 0.615 | 0.287 | 2 | 2,13 |
| J0005.9+3824 | 1.4882 | 38.3375 | FSRQ | 0.273 | 0.071 | 2 | 3,6 |
| J0006.3−0620 | 1.5579 | −6.3931 | BLLAC | 0.391 | 0.296 | 5 | 2,3,6,12a,13 |
| J0006.4+0135 | 1.6122 | 1.6029 | BLLAC | 0.655 | 0.414 | 6 | 1,2,3,6,12c,13 |
| J0007.7+4008 | 1.9236 | 40.1416 | UNCL | - | - | - | |
| J0008.0+4711 | 1.9999 | 47.2022 | BLLAC | 2.324 | - | 1 | 3 |
| J0008.0−3937 | 2.0383 | −39.7564 | UNCL | 1.330 | 0.375 | 3 | 2,4,13 |
| J0008.4+1455 | 2.1058 | 14.9433 | UNCL | 1.075 | - | 1 | 13 |
| J0008.4−2339 | 2.1475 | −23.6578 | BLLAC | 0.150 | - | 1 | 6 |
| J0009.1+0628 | 2.2664 | 6.4726 | BLLAC | 0.682 | 0.428 | 3 | 1,3,13 |
| J0009.3+5030 | 2.3448 | 50.5080 | BLLAC | 0.590 | 0.386 | 2 | 3,4 |
| J0009.7−3217 | 2.3982 | −32.2769 | MIS | 0.017 | 0.001 | 5 | 5,6,12a,12b,13 |
| J0009.8+1340 | 2.4884 | 13.6830 | UNCL | 0.471 | 0.178 | 3 | 1,4,13 |
| J0009.8−4317 | 2.4573 | −43.2806 | BLLAC | 0.200 | 0.060 | 3 | 2,6,13 |
| J0010.6+2043 | 2.6198 | 20.7972 | FSRQ | 0.759 | 0.209 | 3 | 1,3,13 |
| J0010.6−3025 | 2.6489 | −30.4632 | FSRQ | 0.648 | 0.265 | 2 | 2,13 |
| J0010.8−2154 | 2.7235 | −21.9512 | UNCL | 1.169 | - | 1 | 3 |
| J0011.4+0057 | 2.8767 | 0.9644 | FSRQ | 0.734 | 0.408 | 5 | 1,2,3,12c,13 |
| J0011.4−4110 | 2.9683 | −41.0959 | UNCL | 0.834 | 0.221 | 2 | 2,13 |
| J0011.8−3142 | 2.9239 | −31.7058 | UNCL | 0.944 | 0.075 | 2 | 2,13 |
| J0013.1−3955 | 3.2496 | −39.9072 | BLLAC | 0.435 | 0.046 | 2 | 2,13 |
| J0013.4+0950 | 3.3700 | 9.8251 | UNCL | 0.226 | 0.068 | 7 | 4,6,7,8,9,12b,13 |
| J0013.6+4051 | 3.3797 | 40.8603 | MIS | 0.211 | 0.027 | 2 | 3,6 |
| J0013.6−0424 | 3.4755 | −4.3979 | FSRQ | 0.810 | 0.454 | 5 | 1,2,3,12a,13 |
| J0013.9−1854 | 3.4835 | −18.9019 | BLLAC | 0.059 | 0.013 | 3 | 5,6,11 |
| J0014.1+1910 | 3.4849 | 19.1783 | BLLAC | 0.809 | 0.380 | 2 | 3,13 |
| J0014.1−5022 | 3.5478 | −50.3764 | BLLAC | 0.176 | - | 1 | 13 |
| J0014.2+0854 | 3.5822 | 8.9006 | CLAGN | 0.138 | 0.022 | 8 | 5,6,7,8,9,11,12b,13 |
| J0014.3−0500 | 3.5851 | −4.9913 | FSRQ | 0.699 | 0.240 | 4 | 1,2,3,13 |
| J0014.9+3212 | 3.7756 | 32.2704 | UNCL | 0.414 | 0.186 | 5 | 6,7,8,9,13 |
| J0015.2+3537 | 3.8662 | 35.6108 | BLLAC | 0.491 | 0.167 | 3 | 1,3,6 |
| J0015.9+2440 | 4.0151 | 24.6707 | BLLAC | 0.485 | 0.471 | 2 | 3,13 |
| J0016.2−0016 | 4.0462 | −0.2535 | FSRQ | 0.742 | 0.427 | 5 | 1,2,3,6,13 |
| J0016.5+1702 | 3.9166 | 17.0113 | FSRQ | 0.771 | 0.188 | 3 | 1,3,13 |
| J0017.0−0649 | 4.2891 | −6.8426 | UNCL | 0.357 | 0.161 | 5 | 1,2,3,4,13 |
| J0017.5−0514 | 4.3992 | −5.2116 | FSRQ | 0.257 | 0.137 | 4 | 2,3,6,13 |
| J0017.8+1455 | 4.4038 | 14.8505 | BLLAC | 0.557 | 0.585 | 3 | 3,6,13 |
| J0018.4+2946 | 4.6158 | 29.7920 | BLLAC | 0.642 | 0.743 | 4 | 1,3,4,13 |
| J0019.2−5640 | 4.8609 | −56.6951 | UNCL | 0.522 | 0.172 | 2 | 12a,13 |
| J0019.3−8152 | 4.8360 | −81.8809 | BLLAC | - | - | - | |
| J0019.6+2022 | 4.9077 | 20.3627 | BLLAC | 0.775 | 0.108 | 3 | 1,3,13 |
| J0019.6+7327 | 4.9408 | 73.4583 | FSRQ | 1.595 | - | 1 | 3 |
| J0021.0+0322 | 5.2094 | 3.3995 | UNCL | 0.652 | 0.406 | 4 | 1,2,3,13 |
| J0021.5−2552 | 5.3856 | −25.8471 | BLLAC | 0.390 | 0.270 | 4 | 2,3,6,13 |
| J0021.6−0855 | 5.4260 | −9.0123 | BLLAC | 0.436 | 0.105 | 3 | 1,8,13 |
| J0021.9−5140 | 5.5003 | −51.6734 | BLLAC | 0.233 | 0.089 | 2 | 2,13 |
| J0022.0+0006 | 5.5040 | 0.1161 | BLLAC | 0.213 | 0.048 | 9 | 6,7,8,9,11,12a,12b,12c,13 |
| J0022.1−1854 | 5.5386 | −18.8930 | BLLAC | 0.856 | - | 1 | 3 |
| J0022.5+0608 | 5.6352 | 6.1345 | BLLAC | 0.544 | 0.370 | 3 | 1,3,13 |
| J0023.7+4457 | 5.8977 | 44.9433 | FSRQ | 1.092 | - | 1 | 3 |
| J0023.7−6820 | 6.0280 | −68.3485 | MIS | 0.177 | - | 1 | 6 |
| J0023.9+1603 | 6.0053 | 16.0428 | BLLAC | 0.732 | 0.380 | 4 | 1,3,6,13 |
| J0024.4+4647 | 6.0897 | 46.7351 | UNCL | 1.437 | 0.083 | 2 | 3,4 |
| J0024.7+0349 | 6.1884 | 3.8177 | FSRQ | 0.574 | 0.158 | 5 | 1,3,12a,12b,13 |
| J0025.2−2231 | 6.3510 | −22.4632 | FSRQ | 0.940 | - | 1 | 3 |
| J0025.7−4801 | 6.4409 | −48.0653 | UNCL | 0.554 | 0.283 | 2 | 12a,13 |
| J0026.6−4600 | 6.6475 | −46.0197 | BLLAC | - | - | - | |
| J0028.1+7505 | 7.0544 | 75.1036 | UNCL | 1.001 | - | 1 | 3 |
| J0028.4+2001 | 7.1242 | 20.0074 | FSRQ | 0.555 | 0.453 | 3 | 1,3,13 |
| J0028.8−0112 | 7.2541 | −1.2283 | SEY | 0.062 | 0.020 | 10 | 5,6,7,8,9,10,11,12a,12b,13 |
| J0028.9+3553 | 7.2165 | 35.8433 | UNCL | 0.582 | 0.174 | 2 | 1,3 |
| J0029.0−7044 | 7.1732 | −70.7544 | BLLAC | - | - | - | |
| J0029.4+2051 | 7.3692 | 20.8927 | UNCL | 0.257 | 0.056 | 6 | 6,7,8,9,12b,13 |
| J0030.2−1647 | 7.5852 | −16.7870 | BLLAC | 1.954 | - | 1 | 3 |
| J0030.3−4224 | 7.5729 | −42.4129 | FSRQ | 0.321 | 0.156 | 3 | 2,6,13 |
| J0030.6−0212 | 7.6326 | −2.1989 | FSRQ | 0.751 | 0.619 | 4 | 1,2,3,13 |
| J0031.3+0726 | 7.8321 | 7.4149 | BLLAC | 0.828 | 0.926 | 2 | 3,13 |
| J0032.3−5522 | 8.0455 | −55.3744 | UNCL | 1.191 | 0.161 | 2 | 12a,13 |
| J0032.4−2849 | 8.1379 | −28.8223 | BLLAC | 0.169 | 0.040 | 7 | 2,3,6,11,12a,12b,13 |
| J0033.3−2040 | 8.3436 | −20.6523 | BLLAC | 0.073 | 0.018 | 7 | 5,6,7,8,11,12b,13 |
| J0033.5−1921 | 8.3933 | −19.3592 | BLLAC | 0.936 | - | 1 | 3 |
| J0033.9+3858 | 8.5100 | 39.0104 | UNCL | 0.743 | 0.443 | 3 | 1,3,4 |
| J0034.0−4116 | 8.5184 | −41.2721 | UNCL | 1.145 | 0.647 | 3 | 2,4,13 |
| J0035.0−5728 | 8.7644 | −57.4356 | UNCL | 0.272 | 0.115 | 4 | 2,4,6,13 |
| J0035.2+1514 | 8.8114 | 15.2512 | BLLAC | 0.722 | 0.928 | 2 | 11,13 |
| J0035.8−0837 | 8.9427 | −8.5983 | UNCL | 0.965 | 0.290 | 4 | 1,3,4,13 |
| J0036.9+1832 | 9.2475 | 18.5343 | FSRQ | 1.453 | 0.544 | 3 | 1,3,13 |
| J0037.6+3653 | 9.4423 | 36.9864 | FSRQ | 0.207 | 0.070 | 5 | 3,6,7,8,11 |
| J0037.8+1239 | 9.4620 | 12.6389 | BLLAC | 0.062 | 0.015 | 8 | 5,6,7,8,9,11,12b,13 |
| J0037.9+2612 | 9.3298 | 26.2201 | FSRQ | 0.122 | 0.025 | 8 | 5,6,7,8,9,11,12b,13 |
| J0038.1+0012 | 9.5355 | 0.2268 | BLLAC | 0.532 | 0.292 | 4 | 1,2,3,13 |
| J0038.2−2459 | 9.5614 | −24.9840 | FSRQ | 1.141 | 0.805 | 4 | 2,3,12b,13 |
| J0038.7−0204 | 9.5855 | −2.1279 | MIS | 0.199 | 0.036 | 9 | 2,3,6,7,8,9,12a,12b,13 |
| J0039.0−0946 | 9.7762 | −9.7130 | FSRQ | 0.725 | 0.268 | 3 | 1,3,13 |
| J0039.1+4330 | 9.7840 | 43.5041 | UNCL | 0.541 | 0.173 | 3 | 3,4,6 |
| J0039.1−2219 | 9.7842 | −22.3337 | BLLAC | 0.053 | 0.011 | 8 | 5,6,7,8,11,12a,12b,13 |
| J0040.3+4050 | 10.0575 | 40.8346 | BLLAC | 0.295 | 0.127 | 2 | 4,6 |
| J0040.4−2340 | 10.1038 | −23.6669 | BLLAC | 0.178 | 0.044 | 9 | 2,3,6,7,8,11,12a,12b,13 |
| J0040.9+3203 | 10.3164 | 32.1854 | FSRQ | 0.573 | 0.235 | 7 | 3,7,8,9,11,12b,13 |
| J0041.4+3800 | 10.3460 | 37.9822 | FSRQ | 1.110 | 1.004 | 2 | 1,3 |
| J0041.9−4702 | 10.4459 | −47.0269 | BLLAC | 0.138 | 0.029 | 5 | 5,6,12a,12b,13 |
| J0042.0+3640 | 10.5333 | 36.6867 | BLLAC | 0.524 | - | 1 | 3 |
| J0042.2+2319 | 10.5189 | 23.3336 | FSRQ | 0.791 | 0.301 | 3 | 1,3,13 |
| J0043.5−0442 | 10.8922 | −4.7168 | BLLAC | 1.419 | 1.137 | 4 | 1,2,3,13 |
| J0043.6+2223 | 10.8905 | 22.3963 | BLLAC | 0.604 | 0.115 | 3 | 1,3,13 |
| J0043.7−1116 | 10.9528 | −11.2687 | BLLAC | 0.957 | 1.083 | 2 | 3,13 |
| J0043.8+3425 | 10.9535 | 34.4406 | FSRQ | 0.928 | 0.658 | 2 | 1,3 |
| J0044.2−8424 | 11.1112 | −84.3778 | FSRQ | 0.548 | - | 1 | 6 |
| J0045.1−3706 | 11.3003 | −37.0968 | FSRQ | 0.493 | 0.397 | 3 | 2,4,13 |
| J0045.3+2128 | 11.3304 | 21.4611 | BLLAC | 0.115 | - | 1 | 13 |
| J0045.7+1217 | 11.4306 | 12.2866 | BLLAC | 0.163 | 0.051 | 3 | 3,6,13 |
| J0047.1−6203 | 11.8551 | −62.1274 | UNCL | - | - | - | |
| J0047.9+2233 | 12.0109 | 22.5900 | FSRQ | 1.195 | 0.595 | 3 | 1,3,13 |
| J0047.9+3947 | 11.9801 | 39.8160 | BLLAC | 0.155 | 0.029 | 4 | 5,6,7,8 |
| J0048.6−2427 | 12.1541 | −24.4482 | UNCL | 0.365 | 0.378 | 4 | 2,3,4,13 |
| J0049.0+2252 | 12.2557 | 22.8876 | MIS | 0.200 | 0.028 | 7 | 6,7,8,9,11,12b,13 |
| J0049.1+4223 | 12.2465 | 42.3975 | BLLAC | 0.295 | 0.052 | 2 | 7,8 |
| J0049.4−5402 | 12.4535 | −54.0454 | BLLAC | 0.168 | 0.043 | 2 | 2,13 |
| J0049.5−4150 | 12.4123 | −41.8604 | UNCL | 0.286 | 0.079 | 5 | 4,6,12a,12b,13 |
| J0049.6−4500 | 12.3193 | −44.9531 | SEY | 0.255 | 0.311 | 6 | 2,5,6,12a,12b,13 |
| J0049.7+0237 | 12.4301 | 2.6177 | BLLAC | 0.823 | 0.491 | 4 | 1,2,3,13 |
| J0050.0−5736 | 12.4978 | −57.6409 | FSRQ | 0.149 | 0.025 | 3 | 2,6,13 |
| J0050.4−0452 | 12.5897 | −4.8724 | FSRQ | 0.542 | 0.147 | 4 | 1,3,12a,13 |
| J0050.7−0929 | 12.6722 | −9.4848 | BLLAC | 0.020 | - | 1 | 13 |
| J0051.1−0648 | 12.7842 | −6.8340 | FSRQ | 0.767 | 0.379 | 4 | 1,3,6,13 |
| J0051.2−6242 | 12.8194 | −62.7012 | BLLAC | 0.168 | 0.101 | 3 | 2,4,13 |
| J0051.5−4220 | 12.7896 | −42.4426 | FSRQ | 0.780 | 0.654 | 3 | 2,6,13 |
| J0052.9−6644 | 13.2167 | −66.6880 | MIS | - | - | - | |
| J0054.4+8627 | 13.1369 | 86.4623 | UNCL | 0.894 | 0.476 | 3 | 3,4,6 |
| J0054.7−2455 | 13.6948 | −24.9248 | BLLAC | 0.314 | 0.275 | 3 | 2,6,13 |
| J0054.8−1954 | 13.6373 | −19.8836 | UNCL | 1.075 | 0.325 | 3 | 2,3,13 |
| J0055.1−1219 | 13.7991 | −12.2992 | UNCL | 1.343 | 0.381 | 2 | 3,13 |
| J0056.3−0935 | 14.0837 | −9.6083 | MIS | 0.051 | 0.014 | 9 | 5,6,7,8,9,10,11,12b,13 |
| J0056.4−2118 | 14.1345 | −21.2856 | BLLAC | 0.442 | 0.302 | 3 | 2,3,13 |
| J0056.5−3936 | 14.0838 | −39.6957 | AMB | 0.223 | 0.020 | 5 | 5,6,12a,12b,13 |
| J0056.6−4452 | 14.1911 | −44.8506 | BLLAC | 0.386 | 0.181 | 2 | 2,13 |
| J0056.6−5317 | 14.0888 | −53.3131 | UNCL | 0.317 | 0.161 | 3 | 2,4,13 |
| J0056.8+1626 | 14.2304 | 16.4204 | BLLAC | 0.521 | 0.364 | 3 | 1,3,13 |
| J0057.0+4101 | 14.2676 | 40.9987 | UNCL | 0.558 | 0.332 | 3 | 1,3,4 |
| J0057.3+2216 | 14.3888 | 22.3115 | BLLAC | 0.707 | 0.346 | 5 | 3,7,8,9,13 |
| J0057.7+3023 | 14.4537 | 30.3524 | MIS | 0.011 | 0.004 | 6 | 5,6,9,11,12b,13 |
| J0058.0−0539 | 14.5211 | −5.6645 | FSRQ | 0.821 | 0.544 | 4 | 1,2,3,13 |
| J0058.0−3233 | 14.5093 | −32.5724 | BLLAC | 0.321 | 0.240 | 2 | 2,13 |
| J0058.3+1723 | 14.5699 | 17.3871 | UNCL | 0.286 | 0.077 | 6 | 4,7,8,9,12b,13 |
| J0058.4+3315 | 14.6336 | 33.1881 | FSRQ | 0.881 | 0.630 | 2 | 1,3 |
| J0059.2+0006 | 14.7730 | 0.1143 | FSRQ | 0.488 | 0.323 | 3 | 2,3,13 |
| J0059.3−0152 | 14.8205 | −1.8382 | BLLAC | 0.126 | 0.035 | 9 | 5,6,7,8,9,11,12a,12b,13 |
| J0059.5−3338 | 15.0391 | −33.6255 | FSRQ | 0.155 | 0.111 | 3 | 2,12a,13 |
| J0059.5−3512 | 14.8811 | −35.1803 | BLLAC | 0.284 | 0.147 | 4 | 2,4,6,13 |
| J0100.3+0745 | 15.0866 | 7.7643 | BLLAC | 0.983 | 0.916 | 2 | 3,13 |
| J0101.0−0059 | 15.2425 | −0.9299 | BLLAC | 0.545 | 0.220 | 4 | 1,2,3,13 |
| J0101.7−5455 | 15.4242 | −54.9306 | BLLAC | - | - | - | |
| J0101.8−7543 | 15.5778 | −75.7810 | FSRQ | - | - | - | |
| J0102.0+1639 | 15.4905 | 16.6614 | UNCL | 0.549 | 0.221 | 5 | 1,3,4,6,13 |
| J0102.4+0942 | 15.5713 | 9.7360 | BLLAC | 0.306 | 0.228 | 2 | 1,13 |
| J0102.4+4214 | 15.6131 | 42.2386 | NLS1 | 0.458 | 0.015 | 2 | 1,3 |
| J0102.6−5639 | 15.5436 | −56.6179 | UNCL | 0.387 | 0.037 | 2 | 6,13 |
| J0102.7−2001 | 15.7123 | −20.0329 | BLLAC | 0.191 | 0.023 | 5 | 6,11,12a,12b,13 |
| J0103.1+4954 | 15.8154 | 49.9912 | UNCL | 0.833 | 0.177 | 2 | 3,4 |
| J0103.5+1526 | 15.8583 | 15.4402 | BLLAC | 0.175 | 0.026 | 9 | 5,6,7,8,9,10,11,12b,13 |
| J0103.8+1321 | 15.9406 | 13.3959 | BLLAC | 0.299 | 0.209 | 2 | 1,13 |
| J0104.8−2416 | 16.2425 | −24.2746 | FSRQ | 1.101 | 0.476 | 3 | 2,3,13 |
| J0105.1+3929 | 16.2883 | 39.4709 | BLLAC | 1.254 | - | 1 | 3 |
| J0106.9−4832 | 16.7320 | −48.5248 | UNCL | 0.662 | 0.096 | 3 | 12a,12b,13 |
| J0107.3−1210 | 16.7991 | −12.1898 | BLLAC | 0.307 | 0.147 | 5 | 3,6,11,12b,13 |
| J0107.4+0334 | 16.8690 | 3.5635 | BLLAC | 0.870 | 0.419 | 5 | 1,3,6,12b,13 |
| J0108.1−0039 | 17.1118 | −0.6234 | FSRQ | 1.003 | 0.686 | 3 | 2,3,13 |
| J0108.6+0134 | 17.1615 | 1.5834 | FSRQ | 0.507 | 0.342 | 3 | 2,3,13 |
| J0109.1+1815 | 17.2841 | 18.2688 | BLLAC | 0.279 | 0.243 | 2 | 3,13 |
| J0109.3+2401 | 17.3111 | 24.0096 | BLLAC | 0.413 | 0.145 | 5 | 1,3,6,12b,13 |
| J0110.0−4019 | 17.4858 | −40.3475 | BLLAC | 0.166 | 0.041 | 5 | 2,6,12a,12b,13 |
| J0110.2+4151 | 17.5201 | 41.8308 | BLLAC | 0.077 | 0.021 | 5 | 5,6,7,8,11 |
| J0110.7−1254 | 17.7083 | −12.9177 | BLLAC | 0.152 | 0.020 | 4 | 6,11,12b,13 |
| J0111.4+0534 | 17.8758 | 5.6076 | BLLAC | 0.271 | 0.126 | 7 | 3,6,7,8,9,12b,13 |
| J0111.5−2546 | 17.8781 | −25.7587 | UNCL | 1.466 | 0.632 | 3 | 3,4,13 |
| J0112.0−6634 | 18.0788 | −66.5792 | FSRQ | - | - | - | |
| J0112.1+2245 | 18.0243 | 22.7441 | BLLAC | 0.592 | 0.740 | 2 | 3,13 |
| J0112.1−0321 | 18.1631 | −3.4786 | FSRQ | 0.648 | 0.125 | 5 | 1,2,3,12a,13 |
| J0112.6−3158 | 18.1365 | −32.0284 | BLLAC | 0.582 | 0.161 | 4 | 2,4,12a,13 |
| J0112.8+3208 | 18.2097 | 32.1382 | FSRQ | 0.714 | 0.871 | 2 | 3,13 |
| J0112.8−7506 | 18.1307 | −75.1050 | UNCL | 0.300 | - | 1 | 4 |
| J0113.1−3553 | 18.3161 | −35.8634 | FSRQ | 0.389 | 0.386 | 2 | 2,13 |
| J0113.4+4948 | 18.3625 | 49.8067 | FSRQ | 0.624 | 0.433 | 2 | 3,6 |
| J0113.7+0225 | 18.4298 | 2.3715 | BLLAC | 0.037 | 0.005 | 9 | 5,6,7,8,9,11,12a,12b,13 |
| J0114.8+1326 | 18.7199 | 13.4271 | BLLAC | 0.722 | 0.832 | 3 | 3,6,13 |
| J0114.9−3400 | 18.7572 | −34.0076 | BLLAC | 0.214 | 0.069 | 5 | 2,6,12a,12b,13 |
| J0115.1+2622 | 18.7143 | 26.3893 | BLLAC | 1.150 | 0.821 | 4 | 1,3,4,13 |
| J0115.1−0129 | 18.8212 | −1.4513 | FSRQ | 0.895 | 0.612 | 3 | 2,3,13 |
| J0115.6+0356 | 18.9188 | 3.9454 | BLLAC | 0.483 | 0.545 | 3 | 2,3,13 |
| J0115.8+2519 | 18.9423 | 25.3315 | BLLAC | 0.523 | 0.437 | 3 | 3,6,13 |
| J0116.0−1136 | 19.0522 | −11.6043 | FSRQ | 0.469 | 0.411 | 3 | 3,6,13 |
| J0116.0−2745 | 18.9811 | −27.7422 | BLLAC | 0.432 | 0.264 | 3 | 2,3,13 |
| J0116.2−6153 | 19.0817 | −61.8954 | BLLAC | 0.170 | 0.041 | 2 | 2,13 |
| J0116.5−2812 | 19.1544 | −28.1964 | BLLAC | 0.296 | 0.199 | 6 | 2,4,6,12a,12b,13 |
| J0116.5−3046 | 18.9438 | −30.8221 | FSRQ | 1.014 | 0.449 | 2 | 2,13 |
| J0117.5−2442 | 19.4458 | −24.7258 | BLLAC | 0.229 | 0.023 | 5 | 6,11,12a,12b,13 |
| J0117.8−2109 | 19.4533 | −21.1852 | FSRQ | 0.923 | 0.237 | 3 | 3,12a,13 |
| J0118.7−0848 | 19.6841 | −8.8497 | UNCL | 1.645 | 0.470 | 4 | 1,3,4,13 |
| J0118.9−2141 | 19.7386 | −21.6917 | FSRQ | 0.425 | 0.440 | 2 | 3,13 |
| J0119.0−1458 | 19.7692 | −14.9830 | BLLAC | 0.187 | 0.082 | 3 | 2,4,13 |
| J0119.4−5354 | 19.9602 | −53.9550 | UNCL | 0.639 | 0.064 | 3 | 2,4,13 |
| J0119.6+4158 | 20.0115 | 42.0039 | BLLAC | 0.115 | 0.027 | 4 | 3,5,6,11 |
| J0119.9+4053 | 20.0802 | 40.8914 | UNCL | 1.191 | 0.656 | 2 | 1,4 |
| J0120.4−2701 | 20.1319 | −27.0235 | BLLAC | 0.408 | 0.330 | 3 | 2,3,13 |
| J0121.7+5153 | 20.3905 | 51.9310 | UNCL | 0.839 | 0.319 | 2 | 3,4 |
| J0121.8−3916 | 20.4696 | −39.2623 | BLLAC | 0.191 | 0.084 | 5 | 4,6,12a,12b,13 |
| J0122.1−3004 | 20.5150 | −30.0854 | UNCL | 0.567 | 0.025 | 2 | 12a,13 |
| J0123.1+3421 | 20.7860 | 34.3469 | BLLAC | 0.197 | 0.090 | 4 | 6,7,8,9 |
| J0123.7−2311 | 20.9098 | −23.1830 | BLLAC | 0.151 | 0.026 | 5 | 2,6,12a,12b,13 |
| J0124.8−0625 | 21.2104 | −6.4169 | BLLAC | 0.485 | 0.112 | 5 | 1,2,3,6,13 |
| J0125.3−2548 | 21.3285 | −25.8179 | BLLAC | 1.240 | 0.781 | 3 | 2,3,13 |
| J0125.4+3200 | 21.4293 | 31.8873 | UNCL | 1.265 | - | 1 | 13 |
| J0125.7−0015 | 21.3215 | −0.3080 | FSRQ | 1.536 | 0.995 | 5 | 1,2,3,6,13 |
| J0126.0−2221 | 21.5625 | −22.3760 | FSRQ | 0.540 | 0.457 | 4 | 1,2,3,13 |
| J0126.5−1553 | 21.7854 | −15.9317 | UNCL | 0.989 | 0.170 | 4 | 2,3,4,13 |
| J0127.1+3310 | 21.7383 | 33.1250 | BLLAC | 0.524 | 0.153 | 4 | 1,3,4,13 |
| J0127.2+0324 | 21.8081 | 3.3835 | BLLAC | 0.284 | 0.095 | 3 | 2,6,13 |
| J0127.2−0819 | 21.8180 | −8.3580 | BLLAC | 0.419 | 0.226 | 4 | 1,3,8,13 |
| J0127.4−4813 | 21.8118 | −48.2256 | UNCL | 0.866 | - | 1 | 13 |
| J0127.9+4857 | 22.0336 | 49.0183 | AMB | 0.051 | 0.010 | 6 | 3,5,6,7,8,11 |
| J0128.5+4440 | 22.1722 | 44.6550 | FSRQ | 0.398 | 0.082 | 5 | 3,6,7,8,11 |
| J0129.7+3436 | 22.4311 | 34.6163 | AMB | 0.691 | 0.282 | 3 | 1,3,6 |
| J0129.8+1440 | 22.4806 | 14.7800 | FSRQ | 1.188 | 0.489 | 3 | 1,3,13 |
| J0130.6+1844 | 22.6277 | 18.7227 | BLLAC | 0.768 | 0.356 | 3 | 1,3,13 |
| J0132.7−0804 | 23.1714 | −8.0680 | SEY | 0.101 | 0.020 | 9 | 5,6,7,8,9,11,12a,12b,13 |
| J0132.7−1654 | 23.1812 | −16.9135 | FSRQ | 1.185 | 0.814 | 3 | 2,3,13 |
| J0132.8+4324 | 23.1839 | 43.4257 | BLLAC | 1.196 | 0.529 | 4 | 1,3,4,6 |
| J0132.8−4413 | 23.2765 | −44.2393 | BLLAC | 0.151 | 0.042 | 4 | 2,12a,12b,13 |
| J0133.1−5201 | 23.2740 | −52.0011 | FSRQ | 0.043 | - | 1 | 13 |
| J0133.2−4533 | 23.2887 | −45.5900 | UNCL | 0.682 | 0.475 | 4 | 2,6,12a,13 |
| J0134.3−3842 | 23.6335 | −38.7259 | FSRQ | 0.539 | 0.682 | 2 | 2,13 |
| J0134.5+2637 | 23.6175 | 26.6453 | CLAGN | 1.173 | 1.546 | 2 | 3,13 |
| J0135.1+0255 | 23.7793 | 2.9285 | BLLAC | 0.301 | 0.065 | 7 | 6,7,8,9,12a,12b,13 |
| J0136.5+3906 | 24.1358 | 39.0998 | BLLAC | - | - | - | |
| J0137.0+4751 | 24.2441 | 47.8581 | FSRQ | 0.840 | - | 1 | 3 |
| J0137.6−2430 | 24.4098 | −24.5150 | FSRQ | 0.582 | 0.327 | 3 | 2,3,13 |
| J0138.0+2247 | 24.5048 | 22.8024 | BLLAC | 0.715 | 0.878 | 5 | 1,3,4,6,13 |
| J0138.5−4613 | 24.6418 | −46.2376 | BLLAC | 0.076 | 0.017 | 5 | 5,6,12a,12b,13 |
| J0139.0+2601 | 24.7464 | 26.0044 | BLLAC | 0.635 | 0.495 | 3 | 1,3,13 |
| J0140.6+8736 | 24.8016 | 87.6327 | UNCL | 0.777 | 0.590 | 3 | 3,4,6 |
| J0140.6−0758 | 25.1704 | −7.9803 | BLLAC | 0.301 | 0.117 | 5 | 1,2,6,12a,13 |
| J0141.4−0928 | 25.3576 | −9.4788 | BLLAC | 1.167 | 1.133 | 4 | 2,3,4,13 |
| J0142.7−0543 | 25.6620 | −5.7338 | BLLAC | 0.377 | 0.224 | 5 | 1,2,3,6,13 |
| J0143.1−3622 | 25.7865 | −36.3829 | UNCL | 0.865 | - | 1 | 13 |
| J0143.5−3156 | 25.7922 | −32.0157 | FSRQ | 0.386 | 0.076 | 5 | 2,6,12a,12b,13 |
| J0143.7−5846 | 25.9476 | −58.7643 | BLLAC | 0.027 | - | 1 | 13 |
| J0144.6+2705 | 26.1398 | 27.0842 | BLLAC | 0.675 | 0.677 | 2 | 3,13 |
| J0145.0−2732 | 26.2641 | −27.5595 | FSRQ | 0.539 | 0.431 | 4 | 2,3,6,13 |
| J0145.9+2319 | 26.4704 | 23.3220 | BLLAC | 0.922 | 0.266 | 3 | 1,3,13 |
| J0146.0−6746 | 26.4784 | −67.7803 | BLLAC | 0.229 | - | 1 | 6 |
| J0146.3+4606 | 26.6105 | 46.1050 | UNCL | 0.592 | 0.255 | 3 | 3,4,6 |
| J0146.9−5202 | 26.7024 | −52.0427 | BLLAC | 0.060 | 0.009 | 5 | 5,6,12a,12b,13 |
| J0148.6+0127 | 27.1408 | 1.4837 | BLLAC | 0.483 | 0.199 | 4 | 1,2,3,13 |
| J0149.6−0734 | 27.3918 | −7.5548 | UNCL | 0.722 | 0.209 | 5 | 1,2,3,4,13 |
| J0150.6−5448 | 27.6856 | −54.8347 | UNCL | 0.188 | 0.074 | 5 | 2,4,6,12a,13 |
| J0151.0+0539 | 27.7577 | 5.6761 | BLLAC | 0.610 | 0.324 | 4 | 1,3,4,13 |
| J0151.3+8601 | 27.3969 | 86.0210 | BLLAC | 0.168 | 0.062 | 3 | 3,6,11 |
| J0151.4−3607 | 27.8643 | −36.1049 | UNCL | 0.198 | 0.072 | 3 | 2,4,13 |
| J0152.2+2206 | 28.0752 | 22.1188 | FSRQ | 0.898 | 0.294 | 3 | 1,3,13 |
| J0152.2+3714 | 28.0509 | 37.2682 | UNCL | 0.550 | 0.067 | 2 | 3,4 |
| J0152.6+0147 | 28.1650 | 1.7882 | BLLAC | 0.043 | 0.008 | 8 | 5,6,7,8,9,12a,12b,13 |
| J0153.0+7517 | 28.2808 | 75.2953 | UNCL | 2.353 | - | 1 | 3 |
| J0153.5−5107 | 28.5821 | −51.1310 | FSRQ | 0.992 | 0.745 | 2 | 2,13 |
| J0153.9+0823 | 28.5115 | 8.3975 | BLLAC | 0.560 | 0.594 | 2 | 3,13 |
| J0154.3−0236 | 28.5950 | −2.5816 | BLLAC | 0.060 | 0.009 | 9 | 5,6,7,8,9,11,12a,12b,13 |
| J0155.0+4433 | 28.7269 | 44.5605 | BLLAC | 0.856 | - | 1 | 3 |
| J0155.4−0625 | 28.9721 | −6.3595 | UNCL | 0.437 | 0.274 | 7 | 1,2,3,4,6,12c,13 |
| J0156.1+1502 | 29.0004 | 15.0370 | BLLAC | 0.925 | 0.508 | 3 | 1,3,13 |
| J0156.5+3914 | 29.1309 | 39.2419 | FSRQ | 0.629 | 0.305 | 2 | 3,6 |
| J0156.6−1758 | 29.1531 | −18.0172 | UNCL | 0.261 | 0.064 | 8 | 2,3,4,6,11,12a,12b,13 |
| J0156.8−4744 | 29.1918 | −47.7381 | UNCL | 0.117 | 0.023 | 2 | 2,13 |
| J0156.9+4648 | 29.2274 | 46.8085 | UNCL | 0.972 | 0.229 | 2 | 3,4 |
| J0156.9−5301 | 29.2417 | −53.0333 | BLLAC | 0.160 | 0.035 | 5 | 2,6,12a,12b,13 |
| J0157.7−4614 | 29.4630 | −46.2398 | FSRQ | 1.183 | 0.508 | 3 | 2,12b,13 |
| J0158.5−3932 | 29.6588 | −39.5344 | BLLAC | 0.234 | 0.089 | 2 | 2,13 |
| J0158.8+0101 | 29.7199 | 1.0258 | BLLAC | 0.490 | 0.233 | 6 | 1,2,3,8,12c,13 |
| J0159.3−4523 | 29.7780 | −45.2606 | UNCL | 0.812 | 0.283 | 2 | 2,13 |
| J0159.5+1046 | 29.8933 | 10.7849 | BLLAC | 0.120 | 0.013 | 3 | 5,6,13 |
| J0159.7−2740 | 29.9306 | −27.6773 | BLLAC | 0.453 | 0.446 | 3 | 2,3,13 |
| J0200.3−4109 | 30.0875 | −41.1601 | BLLAC | 0.279 | 0.015 | 3 | 2,6,13 |
| J0200.6−6637 | 30.2823 | −66.6369 | FSRQ | - | - | - | |
| J0201.1+0036 | 30.2757 | 0.5667 | BLLAC | 0.157 | 0.062 | 8 | 6,7,8,9,12a,12b,12c,13 |
| J0201.1−4347 | 30.2955 | −43.7820 | UNCL | 0.610 | 0.076 | 5 | 2,4,12a,12b,13 |
| J0202.4+0849 | 30.6101 | 8.8205 | BLLAC | 0.530 | 0.093 | 3 | 1,3,13 |
| J0202.6−0258 | 30.6664 | −3.0355 | FSRQ | 1.047 | 0.223 | 4 | 1,2,3,13 |
| J0202.7+4204 | 30.6819 | 42.0879 | BLLAC | 1.527 | - | 1 | 3 |
| J0202.9−0225 | 30.7176 | −2.3891 | UNCL | 0.142 | 0.082 | 5 | 4,11,12a,12c,13 |
| J0203.6+7233 | 30.8891 | 72.5482 | BLLAC | - | - | - | |
| J0203.7+3042 | 30.9345 | 30.7105 | FSRQ | 0.703 | 0.229 | 3 | 1,3,13 |
| J0204.0−3334 | 31.0533 | −33.5614 | BLLAC | 0.477 | 0.101 | 3 | 6,12a,13 |
| J0204.1−2919 | 31.0440 | −29.3845 | UNCL | 0.740 | 0.122 | 5 | 3,4,12a,12b,13 |
| J0204.3+2417 | 31.0898 | 24.2974 | BLLAC | 0.174 | 0.028 | 8 | 5,6,7,8,9,11,12b,13 |
| J0204.8+1513 | 31.2101 | 15.2364 | FSRQ | 0.779 | 0.097 | 3 | 11,12b,13 |
| J0205.0−1700 | 31.2403 | −17.0222 | FSRQ | 0.923 | 0.711 | 3 | 2,3,13 |
| J0205.2+3212 | 31.2705 | 32.2084 | FSRQ | 0.691 | 0.861 | 2 | 3,13 |
| J0206.4−1151 | 31.6087 | −11.8444 | FSRQ | 0.655 | 0.336 | 4 | 1,2,3,13 |
| J0206.8−5744 | 31.6704 | −57.8303 | UNCL | 0.189 | 0.082 | 2 | 2,13 |
| J0207.4−3855 | 31.8150 | −38.9509 | BLLAC | 0.160 | 0.046 | 4 | 2,5,6,13 |
| J0207.5−1049 | 31.9122 | −10.7968 | UNCL | 0.582 | 0.166 | 6 | 2,3,6,12a,12b,13 |
| J0207.5−2402 | 31.8892 | −24.0339 | UNCL | 0.596 | 0.120 | 4 | 2,3,4,13 |
| J0208.3−6838 | 31.9622 | −68.6320 | BLLAC | - | - | - | |
| J0208.5−0046 | 32.1098 | −0.7956 | BLLAC | 0.684 | 0.236 | 5 | 1,2,3,12c,13 |
| J0208.6+3523 | 32.1590 | 35.3869 | BLLAC | 0.538 | 0.299 | 2 | 3,6 |
| J0209.3+4449 | 32.3214 | 44.8295 | BLLAC | 0.268 | 0.043 | 2 | 4,6 |
| J0209.3−5228 | 32.3401 | −52.4897 | BLLAC | 0.843 | 1.361 | 4 | 2,6,12a,13 |
| J0209.9+7229 | 32.4658 | 72.4907 | FSRQ | 0.101 | - | 1 | 6 |
| J0210.1+2518 | 32.5106 | 25.2905 | UNCL | 0.276 | 0.187 | 3 | 1,4,13 |
| J0210.5−1445 | 32.5966 | −14.7497 | UNCL | 1.112 | 0.218 | 2 | 12a,13 |
| J0210.7−5101 | 32.6925 | −51.0172 | FSRQ | 0.203 | 0.129 | 2 | 2,13 |
| J0211.1−0646 | 32.7914 | −6.7639 | UNCL | 1.264 | 0.030 | 2 | 12c,13 |
| J0211.2+1051 | 32.8049 | 10.8597 | BLLAC | 0.299 | 0.271 | 3 | 3,4,13 |
| J0212.2−0219 | 33.0703 | −2.3655 | BLLAC | 0.169 | 0.059 | 7 | 6,7,8,9,12a,12b,13 |
| J0212.2−2559 | 33.1230 | −25.9718 | UNCL | - | - | - | |
| J0212.4−3502 | 33.1271 | −35.0584 | BLLAC | 0.235 | 0.153 | 2 | 2,13 |
| J0212.8−2721 | 33.2302 | −27.3052 | UNCL | 0.566 | 0.304 | 4 | 2,3,4,13 |
| J0212.9+2244 | 33.2201 | 22.7478 | BLLAC | 0.130 | 0.113 | 2 | 6,13 |
| J0213.8−6949 | 33.4944 | −69.8603 | UNCL | 0.300 | - | 1 | 4 |
| J0214.1−4733 | 33.5409 | −47.5431 | BLLAC | 0.152 | 0.039 | 4 | 6,12a,12b,13 |
| J0214.2−7025 | 33.5186 | −70.4517 | UNCL | 1.200 | - | 1 | 4 |
| J0214.4−5822 | 33.5433 | −58.3686 | UNCL | 0.174 | 0.021 | 7 | 2,4,5,6,12a,12b,13 |
| J0214.6−4333 | 33.6648 | −43.5581 | UNCL | 0.450 | 0.138 | 4 | 6,12a,12b,13 |
| J0214.8−6150 | 33.5675 | −61.8260 | UNCL | 0.735 | 0.420 | 2 | 2,13 |
| J0215.3+7555 | 33.8246 | 75.9147 | UNCL | 0.107 | 0.068 | 3 | 4,5,6 |
| J0215.9+0300 | 34.0019 | 3.0033 | BLLAC | 0.408 | 0.224 | 4 | 1,2,3,13 |
| J0216.5+2313 | 34.1337 | 23.2473 | BLLAC | 0.229 | 0.150 | 3 | 1,6,13 |
| J0216.6−1015 | 34.1620 | −10.2842 | UNCL | 0.737 | 0.379 | 4 | 1,3,4,13 |
| J0216.8+0510 | 34.2318 | 5.1718 | BLLAC | 1.139 | 0.513 | 4 | 1,2,4,13 |
| J0216.8−6635 | 34.2120 | −66.6118 | BLLAC | - | - | - | |
| J0217.0−0821 | 34.2611 | −8.3479 | AMB | 0.444 | 0.218 | 5 | 1,2,3,8,13 |
| J0217.2+0837 | 34.3214 | 8.6177 | BLLAC | 0.479 | 0.539 | 4 | 3,4,6,13 |
| J0217.4+7352 | 34.3784 | 73.8257 | FSRQ | 2.388 | - | 1 | 3 |
| J0217.8+0144 | 34.4540 | 1.7471 | CLAGN | 0.555 | 0.537 | 3 | 2,3,13 |
| J0218.9+3643 | 34.7085 | 36.6785 | UNCL | 1.075 | 0.552 | 3 | 3,4,6 |
| J0218.9−2305 | 34.6676 | −23.1201 | UNCL | 0.685 | 0.120 | 6 | 2,3,4,6,12a,13 |
| J0219.0+2443 | 34.7517 | 24.7557 | BLLAC | 0.489 | 0.476 | 2 | 3,13 |
| J0219.1−1724 | 34.7729 | −17.4203 | BLLAC | 0.113 | 0.038 | 6 | 6,7,8,11,12a,13 |
| J0219.5+0724 | 34.8570 | 7.4596 | BLLAC | 0.934 | 0.455 | 4 | 1,3,6,13 |
| J0220.2+3246 | 35.2002 | 32.6851 | FSRQ | 2.061 | - | 1 | 3 |
| J0220.8−0841 | 35.2019 | −8.7140 | BLLAC | 0.495 | 0.484 | 5 | 1,2,3,6,13 |
| J0221.1+3556 | 35.2729 | 35.9372 | FSRQ | 0.829 | 0.413 | 2 | 3,6 |
| J0221.2−1312 | 35.3012 | −13.0465 | UNCL | 0.851 | 0.165 | 4 | 2,3,4,13 |
| J0221.5+2513 | 35.3624 | 25.2427 | UNCL | 0.543 | 0.247 | 4 | 1,3,4,13 |
| J0221.8+3730 | 35.5644 | 37.5210 | UNCL | 0.923 | - | 1 | 3 |
| J0222.0−1616 | 35.5030 | −16.2546 | FSRQ | 0.543 | 0.064 | 3 | 3,6,13 |
| J0222.6+4302 | 35.6650 | 43.0355 | BLLAC | - | - | - | |
| J0223.0−3447 | 35.7350 | −34.6913 | FSRQ | 0.627 | 0.037 | 2 | 2,13 |
| J0223.1−1117 | 35.8094 | −11.2940 | BLLAC | 0.581 | 0.529 | 3 | 2,3,13 |
| J0223.2−1653 | 35.9324 | −16.9438 | FSRQ | 0.750 | 0.507 | 3 | 2,3,13 |
| J0223.5+3912 | 35.8683 | 39.2142 | UNCL | 1.225 | 0.100 | 2 | 3,4 |
| J0223.5−0928 | 35.9201 | −9.4226 | FSRQ | 0.640 | 0.219 | 5 | 1,2,3,12a,13 |
| J0224.0−1850 | 36.0186 | −18.8423 | UNCL | - | - | - | |
| J0224.0−7941 | 35.9125 | −79.6706 | UNCL | - | - | - | |
| J0224.2+0700 | 36.1185 | 6.9898 | NLS1 | 0.347 | 0.202 | 5 | 3,7,8,9,13 |
| J0224.2+1616 | 36.0493 | 16.2495 | UNCL | 0.887 | 1.002 | 2 | 3,13 |
| J0224.9+1843 | 36.2695 | 18.7802 | FSRQ | 1.379 | 1.570 | 2 | 3,13 |
| J0225.1−2604 | 36.2954 | −26.0552 | UNCL | 0.917 | 0.334 | 4 | 3,4,6,13 |
| J0225.6−4502 | 36.4314 | −45.0546 | UNCL | 0.437 | 0.105 | 4 | 2,6,12b,13 |
| J0225.8+1310 | 36.4639 | 13.1796 | UNCL | 0.466 | 0.390 | 4 | 3,4,6,13 |
| J0226.3−1845 | 36.6985 | −18.7276 | FSRQ | 1.346 | 0.506 | 3 | 2,3,13 |
| J0226.5+0938 | 36.6427 | 9.6456 | UNCL | 0.788 | 0.264 | 2 | 3,13 |
| J0226.5−4441 | 36.6620 | −44.6896 | BLLAC | 0.381 | 0.360 | 2 | 2,13 |
| J0226.6−0553 | 36.6668 | −5.8774 | UNCL | 0.013 | - | 1 | 13 |
| J0226.7+2312 | 36.6303 | 23.1903 | UNCL | 0.373 | 0.087 | 7 | 3,6,7,8,9,12b,13 |
| J0227.2+3928 | 36.7809 | 39.5282 | FSRQ | 1.401 | - | 1 | 3 |
| J0227.3+0201 | 36.8191 | 2.0333 | BLLAC | 0.355 | 0.193 | 6 | 6,7,8,9,12c,13 |
| J0227.8+2246 | 36.9348 | 22.8095 | UNCL | 0.514 | 0.157 | 7 | 3,4,7,8,9,12b,13 |
| J0228.0−3026 | 36.9189 | −30.4343 | FSRQ | 0.354 | 0.046 | 4 | 2,12a,12b,13 |
| J0228.1+8208 | 36.8925 | 82.1088 | UNCL | - | - | - | |
| J0228.2−3102 | 37.0541 | −31.0445 | UNCL | 0.401 | 0.143 | 3 | 2,4,13 |
| J0228.3−5547 | 37.0900 | −55.7676 | FSRQ | 0.557 | 0.077 | 2 | 2,13 |
| J0228.5−2234 | 37.1337 | −22.5642 | UNCL | 0.734 | 0.025 | 4 | 11,12a,12b,13 |
| J0229.5−3644 | 37.3685 | −36.7325 | FSRQ | 0.837 | - | 1 | 13 |
| J0230.8+4032 | 37.6905 | 40.5481 | FSRQ | 0.888 | - | 1 | 3 |
| J0231.2−4745 | 37.7992 | −47.7699 | FSRQ | 0.227 | 0.231 | 2 | 2,13 |
| J0231.2−5754 | 37.7886 | −57.9183 | BLLAC | 0.023 | 0.007 | 4 | 5,6,12b,13 |
| J0231.8+1322 | 37.9412 | 13.3819 | FSRQ | 1.079 | 1.287 | 2 | 3,13 |
| J0232.5−1118 | 38.1746 | −11.3390 | BLLAC | 0.153 | 0.023 | 5 | 5,6,11,12a,13 |
| J0232.8+2018 | 38.2026 | 20.2882 | BLLAC | 0.093 | 0.021 | 8 | 5,6,7,8,9,11,12b,13 |
| J0232.9+2608 | 38.2348 | 26.1619 | UNCL | 0.531 | 0.398 | 3 | 1,3,13 |
| J0233.0+3740 | 38.2833 | 37.7000 | UNCL | 0.127 | 0.034 | 3 | 5,6,11 |
| J0233.5+0654 | 38.3749 | 6.9240 | UNCL | 0.225 | 0.025 | 7 | 6,7,8,9,11,12b,13 |
| J0233.9+8041 | 38.6275 | 80.7270 | UNCL | 1.131 | 0.842 | 2 | 3,4 |
| J0234.3−0628 | 38.5428 | −6.4738 | BLLAC | 0.687 | 0.296 | 5 | 1,2,3,6,13 |
| J0235.6−2939 | 38.9030 | −29.6454 | UNCL | 1.549 | 0.994 | 3 | 2,3,13 |
| J0236.8−6136 | 39.2219 | −61.6042 | FSRQ | 0.350 | 0.108 | 5 | 2,6,12a,12b,13 |
| J0237.6+0923 | 39.4189 | 9.3171 | UNCL | 0.335 | 0.407 | 2 | 3,13 |
| J0237.6−3602 | 39.3919 | −36.0579 | BLLAC | 0.131 | 0.025 | 2 | 2,13 |
| J0237.7+0206 | 39.4082 | 2.1285 | MIS | 0.244 | 0.050 | 9 | 2,3,6,7,8,9,12a,12b,13 |
| J0237.8+2848 | 39.4684 | 28.8025 | FSRQ | 0.565 | 0.658 | 2 | 3,13 |
| J0238.1−3905 | 39.5026 | −39.0846 | UNCL | 0.177 | 0.026 | 6 | 2,4,6,12a,12b,13 |
| J0238.2+1531 | 39.5829 | 15.5563 | UNCL | 0.984 | 0.138 | 2 | 3,13 |
| J0238.4−3116 | 39.6353 | −31.2828 | BLLAC | 0.706 | 1.248 | 5 | 2,5,6,11,13 |
| J0238.6+1637 | 39.6622 | 16.6165 | BLLAC | 0.633 | 0.500 | 2 | 3,13 |
| J0239.5+1326 | 39.8635 | 13.4607 | UNCL | 0.595 | 0.290 | 2 | 3,13 |
| J0239.5−1353 | 39.9130 | −13.9026 | UNCL | 1.274 | 0.741 | 3 | 2,3,13 |
| J0239.7+0415 | 39.9636 | 4.2726 | FSRQ | 0.628 | 0.424 | 4 | 2,3,6,13 |
| J0240.8−3401 | 40.1987 | −34.0063 | UNCL | 0.157 | 0.032 | 3 | 2,4,13 |
| J0241.0−0505 | 40.2341 | −5.0784 | UNCL | 0.536 | 0.202 | 4 | 1,2,3,13 |
| J0241.9−1603 | 40.4642 | −16.0593 | UNCL | 0.455 | 0.176 | 5 | 1,2,3,4,13 |
| J0242.3+1102 | 40.6215 | 11.0169 | FSRQ | 0.863 | 0.176 | 2 | 3,13 |
| J0242.6+1735 | 40.7009 | 17.6168 | UNCL | 1.403 | - | 1 | 13 |
| J0242.9+0045 | 40.7622 | 0.7742 | BLLAC | 0.337 | 0.091 | 7 | 6,7,8,9,12a,12b,13 |
| J0243.2−0550 | 40.8020 | −5.8487 | FSRQ | 1.461 | 0.455 | 5 | 1,2,3,4,13 |
| J0243.4+7119 | 40.8787 | 71.3383 | BLLAC | 0.730 | - | 1 | 3 |
| J0243.7+0321 | 40.9410 | 3.3338 | UNCL | 0.635 | 0.238 | 5 | 2,3,4,6,13 |
| J0244.6−5819 | 41.1679 | −58.3318 | BLLAC | 0.120 | 0.054 | 4 | 5,6,12a,13 |
| J0244.7+1316 | 41.1904 | 13.3353 | FSRQ | 0.693 | 0.644 | 2 | 3,13 |
| J0245.1−0257 | 41.3318 | −2.9412 | BLLAC | 0.373 | 0.235 | 4 | 1,2,3,13 |
| J0245.4+2408 | 41.3202 | 24.0931 | FSRQ | 0.912 | 0.777 | 2 | 3,6 |
| J0245.4−5950 | 41.2207 | −59.8016 | UNCL | 0.512 | 0.083 | 2 | 2,13 |
| J0245.5−4502 | 41.4755 | −44.9943 | FSRQ | 0.136 | 0.088 | 5 | 2,5,6,12a,13 |
| J0245.9−4650 | 41.5005 | −46.8548 | FSRQ | 0.107 | 0.057 | 2 | 2,13 |
| J0246.6−3348 | 41.6945 | −33.8552 | UNCL | - | - | - | |
| J0248.0+2232 | 42.0030 | 22.5220 | UNCL | 0.982 | 0.643 | 2 | 3,4 |
| J0250.2−8224 | 42.7885 | −82.4415 | UNCL | 0.359 | 0.189 | 2 | 4,6 |
| J0250.6+1712 | 42.6582 | 17.2025 | BLLAC | 0.109 | 0.018 | 3 | 5,6,13 |
| J0250.6+8435 | 42.4514 | 84.5992 | UNCL | 0.625 | - | 1 | 3 |
| J0251.5−5958 | 42.8594 | −60.0017 | FSRQ | 0.233 | 0.177 | 2 | 2,13 |
| J0252.8−2219 | 43.1998 | −22.3237 | FSRQ | 1.086 | 0.732 | 2 | 3,13 |
| J0252.9+3834 | 43.2870 | 38.5903 | FSRQ | 0.719 | 0.574 | 2 | 3,6 |
| J0253.2−0124 | 43.3150 | −1.4015 | BLLAC | 0.535 | 0.194 | 4 | 1,2,3,13 |
| J0253.2−5441 | 43.3716 | −54.6976 | FSRQ | 0.299 | 0.269 | 2 | 2,13 |
| J0253.5+3216 | 43.3902 | 32.2891 | FSRQ | 0.992 | - | 1 | 1 |
| J0255.8+0534 | 43.9563 | 5.5653 | BLLAC | 0.580 | 0.214 | 4 | 1,3,8,13 |
| J0256.3+0334 | 44.1173 | 3.5588 | UNCL | 0.971 | 1.140 | 5 | 2,3,4,6,13 |
| J0257.0+3358 | 44.2830 | 33.9584 | UNCL | 0.373 | 0.097 | 2 | 1,4 |
| J0257.9−1215 | 44.4209 | −12.2004 | FSRQ | 0.784 | 0.476 | 3 | 2,3,13 |
| J0258.1+2030 | 44.5305 | 20.5004 | BLLAC | 0.484 | 0.388 | 2 | 3,6 |
| J0259.4+0308 | 44.8560 | 3.1250 | UNCL | 0.275 | 0.104 | 9 | 4,6,7,8,9,11,12a,12b,13 |
| J0259.4+0746 | 44.8628 | 7.7943 | FSRQ | 0.964 | - | 1 | 3 |
| J0259.5+1924 | 44.8736 | 19.4290 | FSRQ | 0.389 | - | 1 | 6 |
| J0259.5−1705 | 44.8892 | −17.0939 | UNCL | 0.629 | 0.192 | 5 | 2,3,4,6,13 |
| J0301.0−1652 | 45.3193 | −16.8792 | BLLAC | 0.374 | 0.403 | 4 | 2,3,6,13 |
| J0301.4−3124 | 45.3177 | −31.4377 | FSRQ | 0.201 | 0.065 | 6 | 2,6,11,12a,12b,13 |
| J0301.6−7155 | 45.4102 | −71.9429 | FSRQ | 0.518 | - | 1 | 6 |
| J0301.9−2731 | 45.4917 | −27.4653 | UNCL | 0.481 | 0.141 | 4 | 2,3,6,13 |
| J0303.2+3149 | 45.7565 | 31.8459 | UNCL | 0.451 | 0.335 | 2 | 3,4 |
| J0303.3+0555 | 45.8758 | 5.9084 | BLLAC | 0.176 | 0.021 | 5 | 5,6,7,8,9 |
| J0303.3−7913 | 45.8371 | −79.2490 | FSRQ | - | - | - | |
| J0303.4−2407 | 45.8604 | −24.1198 | BLLAC | 0.341 | 0.386 | 3 | 3,6,13 |
| J0303.4−5232 | 45.8675 | −52.5759 | UNCL | 0.829 | 0.291 | 3 | 2,4,13 |
| J0303.6−6211 | 45.9610 | −62.1904 | FSRQ | 0.382 | 0.425 | 2 | 2,13 |
| J0304.4−2833 | 46.0680 | −28.5384 | BLLAC | 0.598 | 0.391 | 4 | 2,3,4,13 |
| J0304.5+3349 | 46.1723 | 33.8121 | UNCL | 0.476 | 0.234 | 2 | 3,4 |
| J0304.5−0054 | 46.1415 | −0.9013 | BLLAC | 0.306 | 0.186 | 5 | 1,3,6,8,13 |
| J0304.9−0606 | 46.2523 | −6.1282 | UNCL | 0.880 | 0.213 | 3 | 1,3,13 |
| J0305.1−1608 | 46.3128 | −16.1380 | BLLAC | 0.192 | 0.069 | 7 | 4,6,7,8,12a,12b,13 |
| J0307.8−0419 | 46.9355 | −4.3192 | BLLAC | 0.030 | 0.016 | 5 | 5,6,11,12b,13 |
| J0308.1−2852 | 47.0702 | −28.8514 | UNCL | 0.170 | 0.071 | 6 | 2,4,6,12a,12b,13 |
| J0308.4+0407 | 47.1093 | 4.1109 | MIS | 0.018 | 0.008 | 4 | 5,6,12b,13 |
| J0309.0+1029 | 47.2651 | 10.4879 | FSRQ | 1.398 | - | 1 | 3 |
| J0309.4−4000 | 47.3042 | −40.0308 | BLLAC | 0.164 | 0.014 | 5 | 5,6,12a,12b,13 |
| J0309.7−0745 | 47.4302 | −7.7410 | BLLAC | 0.199 | 0.128 | 7 | 3,6,7,8,9,12b,13 |
| J0309.9−6058 | 47.4837 | −60.9775 | FSRQ | 0.150 | - | 1 | 13 |
| J0310.6−5017 | 47.6447 | −50.2753 | UNCL | 0.239 | 0.071 | 4 | 2,4,6,13 |
| J0310.8−1041 | 47.6421 | −10.6208 | UNCL | 0.177 | 0.041 | 5 | 6,11,12a,12b,13 |
| J0310.9+3815 | 47.7078 | 38.2483 | SEY | 0.576 | - | 1 | 3 |
| J0311.5−4402 | 47.7636 | −44.0411 | UNCL | 0.380 | 0.099 | 3 | 2,4,13 |
| J0311.6+4134 | 47.8856 | 41.5735 | UNCL | 0.558 | 0.195 | 3 | 1,3,4 |
| J0312.5−2221 | 48.1488 | −22.3548 | UNCL | 0.399 | 0.373 | 5 | 2,3,4,6,13 |
| J0312.8+0134 | 48.1817 | 1.5549 | FSRQ | 0.703 | 0.019 | 3 | 1,3,13 |
| J0312.9+3614 | 48.2095 | 36.2554 | BLLAC | 0.054 | 0.007 | 3 | 5,6,11 |
| J0312.9+4119 | 48.2582 | 41.3337 | MIS | 0.133 | 0.046 | 5 | 3,5,6,7,8 |
| J0313.0+0229 | 48.3059 | 2.4765 | FSRQ | 0.744 | 0.017 | 3 | 3,12b,13 |
| J0314.3+0620 | 48.5997 | 6.3324 | BLLAC | 0.143 | - | 1 | 6 |
| J0314.3−5103 | 48.6071 | −51.0754 | BLLAC | 0.258 | 0.189 | 2 | 2,13 |
| J0314.6−6549 | 48.5935 | −65.8069 | FSRQ | 0.377 | 0.392 | 2 | 12a,13 |
| J0315.9−1033 | 48.9870 | −10.5276 | FSRQ | 1.336 | 0.750 | 3 | 2,3,13 |
| J0316.0−5626 | 49.0590 | −56.4322 | UNCL | 0.435 | 0.247 | 2 | 2,13 |
| J0316.2+0905 | 49.0531 | 9.0787 | BLLAC | - | - | - | |
| J0316.2−2608 | 49.0622 | −26.1326 | BLLAC | 0.349 | 0.223 | 4 | 2,3,6,13 |
| J0316.2−6437 | 49.0597 | −64.6254 | BLLAC | 0.211 | 0.119 | 2 | 2,13 |
| J0316.8+4120 | 49.1791 | 41.3249 | MIS | 0.014 | 0.004 | 2 | 5,6 |
| J0316.9−0625 | 49.2709 | −6.4136 | UNCL | 0.533 | 0.136 | 4 | 1,3,4,13 |
| J0317.7−2804 | 49.3904 | −28.0552 | AMB | 1.129 | 0.151 | 3 | 2,3,13 |
| J0317.8−4414 | 49.4903 | −44.2381 | MIS | 0.056 | 0.008 | 5 | 5,6,12a,12b,13 |
| J0318.7+2135 | 49.6903 | 21.5769 | UNCL | 1.830 | - | 1 | 3 |
| J0319.4−7045 | 50.0384 | −70.7593 | UNCL | 0.309 | 0.121 | 2 | 4,6 |
| J0319.8+1845 | 49.9659 | 18.7596 | BLLAC | 0.233 | 0.073 | 3 | 3,6,9 |
| J0319.8+4130 | 49.9507 | 41.5117 | MIS | 0.023 | 0.011 | 2 | 5,11 |
| J0320.6+1125 | 50.1585 | 11.4145 | UNCL | 0.495 | 0.126 | 2 | 3,4 |
| J0321.3+0425 | 50.3780 | 4.4410 | UNCL | 0.781 | 0.525 | 3 | 1,3,4 |
| J0321.3−1612 | 50.2930 | −16.2114 | UNCL | 0.459 | 0.026 | 5 | 6,11,12a,12b,13 |
| J0322.0+2335 | 50.4999 | 23.6031 | BLLAC | 0.427 | - | 1 | 3 |
| J0322.9+0940 | 50.7274 | 9.6840 | UNCL | 1.339 | - | 1 | 3 |
| J0323.7−0111 | 50.9317 | −1.1962 | BLLAC | 0.031 | 0.004 | 2 | 8,13 |
| J0324.3−1313 | 51.1288 | −13.1675 | UNCL | - | - | - | |
| J0324.8+3412 | 51.1715 | 34.1794 | NLS1 | 0.069 | 0.018 | 3 | 3,5,6 |
| J0325.0−2416 | 51.3056 | −24.2633 | FSRQ | 1.112 | 0.085 | 3 | 2,3,13 |
| J0325.3+3332 | 51.3233 | 33.5455 | BLLAC | 0.120 | 0.018 | 3 | 5,6,11 |
| J0325.5−5635 | 51.3480 | −56.5957 | BLLAC | 0.051 | 0.006 | 5 | 5,6,12a,12b,13 |
| J0325.6−1646 | 51.4212 | −16.7713 | BLLAC | 0.138 | 0.083 | 2 | 2,13 |
| J0325.7+2225 | 51.4034 | 22.4001 | FSRQ | 0.810 | - | 1 | 3 |
| J0325.9−1843 | 51.4774 | −18.7366 | UNCL | 0.309 | 0.082 | 7 | 2,3,4,6,12a,12b,13 |
| J0326.2+0225 | 51.5581 | 2.4207 | BLLAC | 0.100 | 0.007 | 3 | 5,6,13 |
| J0326.7−3404 | 51.6839 | −34.0577 | UNCL | - | - | - | |
| J0327.5−1805 | 51.9306 | −18.0617 | FSRQ | 0.831 | 0.147 | 3 | 2,3,13 |
| J0328.8−5715 | 52.2195 | −57.2682 | UNCL | 0.345 | 0.055 | 3 | 2,6,13 |
| J0330.6+0438 | 52.6830 | 4.6680 | UNCL | 0.719 | 0.322 | 3 | 1,3,4 |
| J0331.1−5243 | 52.8125 | −52.6967 | MIS | 0.066 | 0.014 | 5 | 5,6,12a,12b,13 |
| J0331.3−6156 | 52.8270 | −61.9246 | UNCL | 0.141 | 0.032 | 6 | 2,4,5,6,12a,13 |
| J0331.8−7040 | 53.0098 | −70.6636 | BLLAC | 0.192 | - | 1 | 6 |
| J0332.1−1123 | 53.0969 | −11.3307 | FSRQ | 0.313 | 0.202 | 6 | 2,3,6,12a,12b,13 |
| J0332.8+1557 | 53.2168 | 15.9490 | UNCL | 0.934 | 0.731 | 3 | 1,3,4 |
| J0333.1+8227 | 53.0990 | 82.4459 | UNCL | 0.807 | 0.429 | 2 | 3,6 |
| J0333.3+0233 | 53.3400 | 2.5197 | UNCL | 0.863 | - | 1 | 3 |
| J0333.7+2916 | 53.4542 | 29.2754 | BLLAC | - | - | - | |
| J0333.7+7851 | 53.4357 | 78.8413 | UNCL | 0.791 | 0.522 | 2 | 3,4 |
| J0333.8+4007 | 53.4451 | 40.1107 | UNCL | 0.392 | - | 1 | 6 |
| J0334.2−3725 | 53.5643 | −37.4286 | BLLAC | 0.068 | 0.043 | 2 | 2,13 |
| J0334.2−4008 | 53.5569 | −40.1404 | BLLAC | 0.227 | 0.164 | 2 | 2,13 |
| J0334.3+3920 | 53.5767 | 39.3568 | MIS | 0.018 | 0.010 | 3 | 5,6,8 |
| J0335.1−4459 | 53.8078 | −44.9955 | BLLAC | 0.163 | 0.049 | 2 | 2,13 |
| J0336.4+3224 | 54.1254 | 32.3082 | FSRQ | 0.810 | 0.965 | 2 | 3,6 |
| J0336.5−0348 | 54.0992 | −3.7941 | BLLAC | 0.137 | 0.019 | 5 | 5,6,11,12b,13 |
| J0336.8−3612 | 54.2251 | −36.2684 | FSRQ | 0.725 | 0.900 | 2 | 2,13 |
| J0337.8−1157 | 54.4810 | −12.0679 | FSRQ | 1.008 | 0.390 | 2 | 2,13 |
| J0338.1−2443 | 54.5521 | −24.7306 | BLLAC | 0.228 | 0.042 | 5 | 6,11,12a,12b,13 |
| J0338.5+1302 | 54.6220 | 13.0376 | BLLAC | 1.871 | - | 1 | 3 |
| J0338.7−5706 | 54.6334 | −57.0802 | BLLAC | 0.239 | 0.058 | 5 | 4,6,12a,12b,13 |
| J0339.2−1736 | 54.8071 | −17.6002 | MIS | 0.040 | 0.009 | 6 | 5,6,11,12a,12b,13 |
| J0339.5−0146 | 54.8789 | −1.7766 | FSRQ | 0.630 | 0.722 | 2 | 3,13 |
| J0340.4−2422 | 55.0954 | −24.4020 | FSRQ | 0.964 | 0.717 | 5 | 2,3,4,6,13 |
| J0340.5−0256 | 55.1358 | −2.9151 | UNCL | 0.619 | 0.153 | 5 | 3,4,6,12b,13 |
| J0340.5−2118 | 55.1484 | −21.3253 | BLLAC | 0.403 | 0.254 | 3 | 2,3,13 |
| J0342.2+3858 | 55.5678 | 38.9851 | FSRQ | 1.189 | 0.486 | 3 | 1,3,6 |
| J0342.8−3007 | 55.6681 | −30.1328 | UNCL | 0.866 | 0.148 | 4 | 4,11,12a,13 |
| J0343.2−2529 | 55.8313 | −25.5048 | FSRQ | 0.942 | 0.581 | 4 | 2,3,6,13 |
| J0343.2−6444 | 55.8359 | −64.7154 | UNCL | 0.582 | 0.791 | 4 | 2,6,12a,13 |
| J0343.4+3621 | 55.8706 | 36.3701 | FSRQ | 1.453 | 0.009 | 2 | 1,3 |
| J0344.2+3203c | 56.0758 | 32.1510 | UNCL | - | - | - | |
| J0344.4+3432 | 56.1040 | 34.5050 | UNCL | 0.251 | - | 1 | 6 |
| J0345.2−2353 | 56.3263 | −23.8723 | BLLAC | 0.526 | 0.441 | 4 | 2,3,12a,13 |
| J0345.5−3301 | 56.3740 | −32.9354 | UNCL | 0.522 | 0.193 | 5 | 4,6,12a,12b,13 |
| J0347.7−3616 | 56.9962 | −36.2768 | UNCL | 0.761 | 0.082 | 2 | 2,13 |
| J0348.5−2749 | 57.1589 | −27.8204 | FSRQ | 0.605 | 0.242 | 3 | 2,3,13 |
| J0348.6−1609 | 57.1636 | −16.1716 | BLLAC | 0.437 | 0.438 | 4 | 2,3,6,13 |
| J0348.8−0828 | 57.1901 | −8.4069 | UNCL | 1.140 | 0.611 | 3 | 3,4,13 |
| J0348.9−4859 | 57.3039 | −48.9736 | UNCL | 0.583 | 0.147 | 6 | 2,4,6,12a,12b,13 |
| J0349.4−1159 | 57.3466 | −11.9909 | AMB | 0.159 | 0.068 | 5 | 6,7,8,12b,13 |
| J0349.6+2410 | 57.4304 | 24.2533 | UNCL | - | - | - | |
| J0349.8−2103 | 57.4909 | −21.0466 | FSRQ | 1.024 | 0.072 | 3 | 2,3,13 |
| J0350.0+0640 | 57.4910 | 6.6906 | UNCL | 0.206 | 0.070 | 3 | 4,6,11 |
| J0350.4−5144 | 57.6182 | −51.7484 | UNCL | 0.275 | 0.044 | 3 | 2,4,6 |
| J0350.6−3226 | 57.6805 | −32.5498 | FSRQ | 1.088 | 0.018 | 3 | 12a,12b,13 |
| J0350.8−2814 | 57.7138 | −28.2758 | UNCL | 0.685 | 0.212 | 4 | 2,3,4,13 |
| J0352.0−2516 | 58.0461 | −25.2473 | UNCL | 0.606 | 0.187 | 4 | 2,3,6,13 |
| J0352.9−3623 | 58.2712 | −36.3856 | BLLAC | 1.209 | 1.410 | 3 | 2,4,13 |
| J0353.0−6831 | 58.2400 | −68.5214 | MIS | 0.056 | 0.002 | 2 | 5,6 |
| J0353.7+8257 | 58.2855 | 82.9421 | BLLAC | 0.068 | 0.015 | 3 | 5,6,11 |
| J0354.7+8009 | 58.6922 | 80.1580 | BLLAC | 0.744 | 0.460 | 2 | 1,3 |
| J0354.7−1617 | 58.6043 | −16.2729 | FSRQ | 0.910 | 0.282 | 3 | 2,3,13 |
| J0355.3+3909 | 58.8191 | 39.1527 | UNCL | 0.846 | 0.595 | 2 | 3,4 |
| J0356.1−1329 | 59.0454 | −13.4850 | UNCL | 0.234 | 0.092 | 6 | 2,4,6,12a,12b,13 |
| J0357.0−4955 | 59.2508 | −49.9302 | BLLAC | 0.254 | 0.195 | 2 | 2,13 |
| J0357.2+2320 | 59.3400 | 23.3316 | UNCL | 1.250 | - | 1 | 3 |
| J0357.2−0319 | 59.3588 | −3.2999 | UNCL | 0.239 | 0.036 | 4 | 4,6,12b,13 |
| J0357.6−4625 | 59.3697 | −46.4287 | BLLAC | 0.080 | 0.012 | 5 | 4,5,6,12b,13 |
| J0358.0−6946 | 59.3753 | −69.8125 | UNCL | - | - | - | |
| J0358.1−5954 | 59.5583 | −59.8759 | UNCL | 0.488 | 0.004 | 2 | 12b,13 |
| J0358.6+0634 | 59.6131 | 6.4887 | UNCL | 0.654 | 0.206 | 2 | 3,4 |
| J0358.7+7649 | 59.6263 | 76.8242 | UNCL | 0.662 | 0.423 | 2 | 3,6 |
| J0359.0−3053 | 59.7342 | −30.9128 | BLLAC | 0.136 | - | 1 | 13 |
| J0359.4−2616 | 59.8903 | −26.2587 | BLLAC | 0.886 | 0.259 | 3 | 2,3,13 |
| J0400.7+3920 | 60.1891 | 39.3527 | UNCL | 1.100 | - | 1 | 3 |
| J0401.0−5353 | 60.2967 | −53.9162 | UNCL | 0.489 | 0.130 | 3 | 4,12a,13 |
| J0401.3+0412 | 60.3330 | 4.2262 | BLLAC | 0.568 | - | 1 | 3 |
| J0401.7+2112 | 60.4382 | 21.1746 | FSRQ | 1.010 | - | 1 | 3 |
| J0401.9−2034 | 60.4696 | −20.5861 | UNCL | 0.626 | 0.137 | 3 | 3,4,13 |
| J0402.0+2737 | 60.5133 | 27.6211 | UNCL | 1.274 | - | 1 | 3 |
| J0402.0−2616 | 60.5033 | −26.2609 | BLLAC | 0.407 | 0.289 | 3 | 2,3,13 |
| J0402.1−3147 | 60.5886 | −31.7905 | FSRQ | 0.487 | 0.250 | 2 | 2,13 |
| J0403.3+2601 | 60.7733 | 26.0004 | FSRQ | 0.762 | 0.288 | 2 | 3,6 |
| J0403.5−2437 | 60.9239 | −24.7357 | FSRQ | 0.483 | 0.159 | 3 | 2,3,13 |
| J0403.9−3605 | 60.9740 | −36.0839 | FSRQ | 0.177 | 0.165 | 2 | 2,13 |
| J0404.1−1715 | 61.1070 | −17.3074 | UNCL | 0.554 | 0.378 | 4 | 2,3,4,13 |
| J0404.3−1559 | 61.1737 | −15.9905 | UNCL | 1.223 | 0.411 | 3 | 3,4,13 |
| J0405.6−1308 | 61.3917 | −13.1371 | FSRQ | 0.365 | 0.433 | 2 | 3,13 |
| J0406.0−5407 | 61.5361 | −54.0805 | BLLAC | 0.193 | 0.025 | 5 | 2,6,12a,12b,13 |
| J0407.0−3826 | 61.7460 | −38.4411 | FSRQ | 0.350 | 0.334 | 2 | 2,13 |
| J0407.5+0741 | 61.8712 | 7.7021 | CLAGN | 0.478 | 0.423 | 2 | 3,6 |
| J0409.4+3201 | 62.3684 | 32.0460 | UNCL | 0.243 | 0.076 | 2 | 4,6 |
| J0409.8−0359 | 62.4441 | −4.0010 | BLLAC | 0.666 | 0.666 | 2 | 3,13 |
| J0411.7+3041 | 62.9436 | 30.6632 | UNCL | - | - | - | |
| J0412.3+0239 | 63.1196 | 2.6772 | UNCL | 0.834 | 0.178 | 2 | 3,4 |
| J0413.1−5332 | 63.3061 | −53.5335 | FSRQ | 0.895 | - | 1 | 13 |
| J0414.6−0842 | 63.6379 | −8.7019 | BLLAC | 0.735 | 0.430 | 2 | 3,13 |
| J0414.8−5338 | 63.7422 | −53.6622 | BLLAC | 0.825 | 0.904 | 3 | 2,6,13 |
| J0415.2−5741 | 63.7774 | −57.7065 | UNCL | 0.698 | 0.096 | 2 | 12a,13 |
| J0416.0−4743 | 63.9761 | −47.6265 | UNCL | 0.475 | 0.074 | 3 | 2,4,13 |
| J0416.0−6628 | 64.0217 | −66.4826 | BLLAC | 0.219 | - | 1 | 6 |
| J0416.2−4353 | 64.0553 | −43.8489 | UNCL | 1.044 | - | 1 | 13 |
| J0416.5−1852 | 64.1523 | −18.8523 | FSRQ | 0.830 | 0.353 | 3 | 2,3,13 |
| J0416.9+0105 | 64.2187 | 1.0900 | BLLAC | 0.088 | - | 1 | 6 |
| J0418.1−0252 | 64.4928 | −2.8387 | UNCL | 0.125 | - | 1 | 13 |
| J0418.4+3414 | 64.5415 | 34.1930 | UNCL | 1.256 | 0.727 | 3 | 1,3,4 |
| J0420.0+0805 | 64.9967 | 8.0774 | UNCL | 1.143 | 0.105 | 3 | 1,3,4 |
| J0420.3−3745 | 65.1046 | −37.7458 | UNCL | 0.257 | 0.121 | 4 | 2,4,12a,13 |
| J0420.3−6016 | 65.0460 | −60.2514 | UNCL | 0.225 | 0.100 | 2 | 2,4 |
| J0421.0−0752 | 65.2248 | −7.8722 | UNCL | 0.193 | 0.025 | 4 | 5,6,12b,13 |
| J0422.1−0644 | 65.5450 | −6.7293 | FSRQ | 0.336 | 0.326 | 4 | 3,6,11,13 |
| J0422.3+1951 | 65.5771 | 19.8481 | BLLAC | - | - | - | |
| J0422.8+0225 | 65.7176 | 2.3241 | FSRQ | 1.337 | 1.081 | 2 | 3,6 |
| J0423.1+2106 | 65.7583 | 21.1339 | UNCL | 0.649 | 0.236 | 3 | 1,3,4 |
| J0423.3−0120 | 65.8158 | −1.3425 | FSRQ | 0.344 | 0.346 | 2 | 3,13 |
| J0424.7+0036 | 66.1952 | 0.6018 | BLLAC | 0.793 | 1.004 | 2 | 3,13 |
| J0424.9−5331 | 66.2678 | −53.5328 | BLLAC | 0.175 | 0.033 | 2 | 2,13 |
| J0426.7+6826 | 66.7086 | 68.4314 | UNCL | 0.581 | 0.440 | 2 | 3,6 |
| J0427.3−3900 | 66.8403 | −39.0167 | UNCL | 0.718 | 0.272 | 3 | 2,4,13 |
| J0428.6−3756 | 67.1684 | −37.9388 | BLLAC | 0.180 | 0.094 | 2 | 2,13 |
| J0428.7−5003 | 67.1776 | −50.0929 | UNCL | 1.328 | 0.296 | 2 | 2,13 |
| J0429.0−0006 | 67.3297 | −0.1030 | UNCL | 1.056 | 0.135 | 3 | 3,4,13 |
| J0429.3−3238 | 67.2508 | −32.6108 | BLLAC | 1.105 | - | 1 | 13 |
| J0429.3−4326 | 67.3543 | −43.4768 | FSRQ | 0.731 | 0.511 | 3 | 2,6,13 |
| J0429.8+2843 | 67.4583 | 28.7148 | UNCL | 1.232 | 0.843 | 2 | 3,4 |
| J0429.9−3101 | 67.4956 | −30.9931 | BLLAC | 0.138 | 0.044 | 3 | 6,12a,13 |
| J0430.2−0356 | 67.8670 | −4.1075 | FSRQ | 0.660 | 0.263 | 5 | 1,3,6,11,13 |
| J0430.3+1654 | 67.5931 | 16.9180 | UNCL | 0.758 | 0.612 | 2 | 3,4 |
| J0430.3−2507 | 67.5668 | −25.1275 | BLLAC | 0.563 | 0.400 | 4 | 2,3,6,13 |
| J0431.8+7403 | 67.9378 | 74.0574 | BLLAC | 1.352 | - | 1 | 3 |
| J0432.0+1732 | 67.9891 | 17.5266 | BLLAC | 1.227 | - | 1 | 3 |
| J0433.0+0522 | 68.2962 | 5.3543 | MIS | 0.344 | 0.420 | 3 | 3,5,6 |
| J0433.1+3227 | 68.2815 | 32.4780 | BLLAC | - | - | - | |
| J0433.5−1039 | 68.3870 | −10.7090 | UNCL | 0.217 | 0.048 | 4 | 4,6,12b,13 |
| J0433.6+2905 | 68.4076 | 29.0987 | BLLAC | 0.655 | 0.802 | 2 | 3,6 |
| J0433.6−6030 | 68.3921 | −60.5038 | FSRQ | 0.687 | - | 1 | 13 |
| J0433.7−5725 | 68.4339 | −57.4370 | BLLAC | 0.421 | 0.098 | 3 | 2,6,13 |
| J0434.1−2014 | 68.5330 | −20.2548 | BLLAC | 0.731 | 0.166 | 3 | 2,3,13 |
| J0434.4−2342 | 68.6207 | −23.7015 | BLLAC | 0.979 | 0.344 | 2 | 3,13 |
| J0434.7+0922 | 68.6708 | 9.3969 | BLLAC | 0.882 | 0.910 | 2 | 3,4 |
| J0435.4−2623 | 68.8240 | −26.3562 | BLLAC | 0.202 | 0.083 | 4 | 2,12a,12b,13 |
| J0436.7−7148 | 69.2682 | −71.8056 | UNCL | 0.800 | - | 1 | 4 |
| J0436.8−5223 | 69.2175 | −52.2776 | UNCL | 0.618 | 0.135 | 5 | 2,4,12a,12b,13 |
| J0437.2−5846 | 69.1801 | −58.6695 | UNCL | 0.307 | - | 1 | 13 |
| J0437.4−6155 | 69.3324 | −61.9486 | BLLAC | - | - | - | |
| J0438.4−1254 | 69.6459 | −12.8509 | FSRQ | 0.704 | 0.259 | 2 | 3,6 |
| J0438.7−3441 | 69.6867 | −34.6970 | AMB | 0.383 | 0.023 | 2 | 4,6 |
| J0438.9−4521 | 69.7536 | −45.3729 | BLLAC | 0.678 | 0.029 | 2 | 2,13 |
| J0439.2+2151 | 69.7329 | 21.8862 | UNCL | 1.270 | 0.039 | 2 | 1,4 |
| J0439.4−3202 | 69.8842 | −32.0145 | UNCL | 0.343 | 0.048 | 4 | 2,4,6,13 |
| J0439.8−1859 | 69.9572 | −19.0171 | UNCL | 0.708 | 0.565 | 3 | 2,3,13 |
| J0440.2−2458 | 70.0776 | −24.9926 | BLLAC | 0.324 | 0.148 | 5 | 4,6,12a,12b,13 |
| J0440.3−4333 | 70.0716 | −43.5524 | FSRQ | 0.451 | 0.001 | 2 | 2,13 |
| J0440.4+1440 | 70.0881 | 14.6325 | UNCL | 1.115 | - | 1 | 3 |
| J0440.8+2749 | 70.2099 | 27.8464 | BLLAC | 0.200 | - | 1 | 4 |
| J0441.3−2617 | 70.3338 | −26.2833 | UNCL | 1.249 | 0.737 | 3 | 4,12a,13 |
| J0441.5+1505 | 70.3642 | 15.0822 | BLLAC | 0.421 | 0.341 | 2 | 3,6 |
| J0442.6−0017 | 70.6611 | −0.2954 | NLS1 | 0.644 | 0.210 | 3 | 1,3,13 |
| J0442.7+6142 | 70.6694 | 61.6776 | UNCL | 0.200 | - | 1 | 4 |
| J0443.3−6652 | 70.8258 | −66.8679 | FSRQ | - | - | - | |
| J0443.4−4152 | 70.8683 | −41.8656 | BLLAC | 0.314 | 0.239 | 3 | 2,6,13 |
| J0444.5+0719 | 71.0915 | 7.2883 | UNCL | 0.845 | 0.193 | 2 | 3,11 |
| J0445.1−6012 | 71.2563 | −60.2499 | FSRQ | 0.098 | 0.018 | 5 | 5,6,12a,12b,13 |
| J0447.2−2539 | 71.8394 | −25.6585 | UNCL | 0.166 | 0.051 | 6 | 4,6,11,12a,12b,13 |
| J0447.4−2747 | 71.8172 | −27.8019 | UNCL | 1.105 | 0.035 | 4 | 2,12a,12b,13 |
| J0448.6−1632 | 72.1568 | −16.5453 | BLLAC | 1.768 | - | 1 | 3 |
| J0449.1+1121 | 72.2820 | 11.3579 | CLAGN | 0.897 | 0.652 | 2 | 1,3 |
| J0449.2+6329 | 72.3471 | 63.5360 | FSRQ | 0.829 | 0.441 | 2 | 3,6 |
| J0449.4−4350 | 72.3529 | −43.8358 | BLLAC | 0.037 | - | 1 | 13 |
| J0449.6−8100 | 72.5227 | −81.0173 | FSRQ | 0.330 | - | 1 | 6 |
| J0450.3−4419 | 72.5088 | −44.3059 | UNCL | 0.743 | 0.102 | 3 | 2,4,13 |
| J0450.4+7230 | 72.7904 | 72.5035 | UNCL | 0.552 | 0.252 | 3 | 3,4,6 |
| J0450.7−4938 | 72.7612 | −49.6074 | UNCL | 0.749 | 0.198 | 2 | 4,13 |
| J0451.8−4651 | 72.9723 | −46.8889 | FSRQ | 0.722 | 0.171 | 2 | 6,13 |
| J0452.0+2100 | 73.0638 | 21.0511 | UNCL | 0.417 | 0.279 | 3 | 3,4,6 |
| J0453.1+6322 | 73.3019 | 63.3550 | UNCL | 2.099 | - | 1 | 3 |
| J0453.1−2806 | 73.3110 | −28.1270 | FSRQ | 0.586 | 0.405 | 3 | 2,3,13 |
| J0455.7−4617 | 73.9616 | −46.2663 | FSRQ | 0.491 | 0.612 | 2 | 2,13 |
| J0456.2+2702 | 74.0724 | 27.0392 | UNCL | - | - | - | |
| J0456.4−4043 | 74.1346 | −40.6895 | UNCL | 0.606 | 0.067 | 4 | 6,12a,12b,13 |
| J0456.6−3136 | 74.1528 | −31.6035 | FSRQ | 0.449 | 0.139 | 4 | 2,6,11,13 |
| J0457.0+0646 | 74.2821 | 6.7520 | FSRQ | 0.536 | 0.271 | 2 | 3,6 |
| J0457.0−2324 | 74.2632 | −23.4145 | BLLAC | 0.624 | 0.664 | 3 | 2,3,13 |
| J0458.0+1152 | 74.5204 | 11.8620 | UNCL | 0.152 | 0.042 | 6 | 4,5,6,7,8,11 |
| J0459.4+1921 | 74.8646 | 19.3709 | UNCL | 0.385 | 0.184 | 2 | 3,6 |
| J0500.6−4911 | 75.1617 | −49.2046 | UNCL | 0.194 | 0.088 | 5 | 2,6,12a,12b,13 |
| J0501.0+2424 | 75.2788 | 24.3884 | UNCL | 0.839 | 0.718 | 2 | 3,4 |
| J0501.2−0158 | 75.3034 | −1.9873 | FSRQ | 0.775 | 0.486 | 2 | 3,6 |
| J0502.4+0609 | 75.5644 | 6.1521 | FSRQ | 1.214 | - | 1 | 3 |
| J0502.5+1340 | 75.6384 | 13.6364 | BLLAC | 0.635 | 0.407 | 2 | 3,6 |
| J0502.9+6533 | 75.7742 | 65.5670 | UNCL | 0.240 | 0.080 | 2 | 4,6 |
| J0503.1−6045 | 76.0071 | −60.8313 | FSRQ | 0.956 | 0.059 | 2 | 2,13 |
| J0503.5−1116 | 75.8971 | −11.2519 | BLLAC | 2.264 | - | 1 | 3 |
| J0505.3+0459 | 76.3466 | 4.9952 | FSRQ | 0.947 | - | 1 | 3 |
| J0505.6+0415 | 76.3949 | 4.2652 | BLLAC | 0.143 | - | 1 | 6 |
| J0505.6+6405 | 76.4206 | 64.1073 | UNCL | 1.270 | 0.707 | 2 | 3,4 |
| J0505.6−1558 | 76.4233 | −15.9773 | UNCL | 0.415 | 0.137 | 2 | 3,6 |
| J0505.8−0419 | 76.4635 | −4.3241 | FSRQ | 0.496 | 0.095 | 2 | 1,3 |
| J0505.8−3817 | 76.5070 | −38.3488 | BLLAC | 0.137 | 0.012 | 5 | 5,6,12a,12b,13 |
| J0506.0+6113 | 76.4949 | 61.2267 | BLLAC | 0.300 | - | 1 | 4 |
| J0506.0−0357c | 76.5249 | −4.0312 | BLLAC | 1.221 | 1.034 | 2 | 1,3 |
| J0506.7−0857 | 76.6663 | −8.9672 | UNCL | 0.486 | 0.248 | 2 | 3,4 |
| J0506.9+0323 | 76.7089 | 3.3997 | BLLAC | 0.593 | 0.447 | 3 | 3,4,6 |
| J0506.9−5435 | 76.7409 | −54.5844 | BLLAC | 0.102 | 0.002 | 2 | 2,13 |
| J0507.4−3346 | 76.8636 | −33.7765 | BLLAC | 0.288 | 0.174 | 3 | 2,12a,13 |
| J0507.7−6104 | 76.9778 | −61.0786 | FSRQ | 0.677 | - | 1 | 13 |
| J0507.9+6737 | 76.9840 | 67.6234 | BLLAC | - | - | - | |
| J0508.2−1937 | 77.0792 | −19.5989 | FSRQ | 1.170 | 0.408 | 3 | 2,3,13 |
| J0509.1+1943 | 77.3254 | 19.6918 | UNCL | 0.577 | - | 1 | 11 |
| J0509.4+0542 | 77.3582 | 5.6931 | BLLAC | 0.842 | - | 1 | 3 |
| J0509.4+1012 | 77.3644 | 10.1957 | CLAGN | 0.590 | 0.545 | 2 | 3,6 |
| J0509.6+8425 | 77.1765 | 84.5346 | BLLAC | 0.621 | - | 1 | 3 |
| J0509.6−0402 | 77.4091 | −4.0127 | UNCL | 0.144 | - | 1 | 6 |
| J0509.9−6417 | 77.4887 | −64.2949 | BLLAC | - | - | - | |
| J0510.0+1800 | 77.5099 | 18.0116 | CLAGN | 0.537 | 0.357 | 2 | 3,6 |
| J0510.4−1809 | 77.5639 | −18.2078 | UNCL | 1.117 | 0.853 | 2 | 3,13 |
| J0511.4−6804 | 77.8732 | −68.1048 | UNCL | - | - | - | |
| J0513.9−3746 | 78.5167 | −37.7680 | UNCL | 0.793 | 0.142 | 2 | 4,13 |
| J0514.5+6247 | 78.5901 | 62.7443 | UNCL | 0.169 | - | 1 | 6 |
| J0515.5−0125 | 78.9010 | −1.4078 | UNCL | 1.164 | 0.247 | 4 | 1,3,4,6 |
| J0515.6−4556 | 78.9385 | −45.9453 | AMB | 0.184 | 0.136 | 4 | 2,6,12a,13 |
| J0515.8+1527 | 78.9473 | 15.4546 | BLLAC | 0.648 | 0.502 | 2 | 3,6 |
| J0515.9+0537 | 78.9654 | 5.5501 | UNCL | - | - | - | |
| J0516.1−7240 | 79.1572 | −72.6187 | UNCL | 0.536 | - | 1 | 6 |
| J0516.4+7350 | 79.1301 | 73.8524 | BLLAC | - | - | - | |
| J0516.7−6207 | 79.1872 | −62.1182 | BLLAC | 1.039 | 0.672 | 3 | 2,4,13 |
| J0516.8−0509 | 79.3671 | −5.3447 | FSRQ | 1.530 | 0.308 | 2 | 1,3 |
| J0517.5+0858 | 79.4169 | 8.9766 | FSRQ | 0.400 | 0.135 | 3 | 3,6,11 |
| J0517.7−1758 | 79.3502 | −17.9400 | UNCL | 0.952 | 0.197 | 3 | 11,12b,13 |
| J0519.0+0851 | 79.7950 | 8.8158 | UNCL | 1.268 | - | 1 | 3 |
| J0519.6−4544 | 79.9572 | −45.7788 | MIS | 0.127 | 0.145 | 6 | 2,5,6,12a,12b,13 |
| J0521.2+1637 | 80.2912 | 16.6395 | MIS | 0.791 | 0.017 | 2 | 1,3 |
| J0521.3−1734 | 80.3482 | −17.6251 | FSRQ | 0.269 | 0.150 | 6 | 2,3,6,12a,12b,13 |
| J0521.6+0103 | 80.4200 | 1.0488 | BLLAC | 1.536 | - | 1 | 3 |
| J0521.8−3848 | 80.4553 | −38.8419 | UNCL | 0.428 | 0.213 | 4 | 4,6,12a,13 |
| J0522.9−3628 | 80.7416 | −36.4586 | CLAGN | 0.125 | 0.164 | 5 | 2,6,12a,12b,13 |
| J0524.6−2819 | 81.2276 | −28.3116 | UNCL | 1.042 | 0.366 | 3 | 2,3,13 |
| J0525.4−4600 | 81.3808 | −45.9652 | FSRQ | 0.696 | 0.873 | 2 | 2,13 |
| J0525.6−2008 | 81.3668 | −20.1801 | BLLAC | 0.066 | 0.012 | 3 | 11,12a,13 |
| J0525.6−6013 | 81.4268 | −60.2278 | UNCL | 0.637 | 0.102 | 4 | 2,4,6,13 |
| J0525.8−0052 | 81.4776 | −0.8612 | UNCL | 0.704 | 0.351 | 3 | 1,3,4 |
| J0526.1+6318 | 81.5280 | 63.2914 | UNCL | 1.301 | - | 1 | 3 |
| J0526.2−4830 | 81.5695 | −48.5102 | FSRQ | 0.587 | 0.551 | 2 | 2,13 |
| J0526.7−1519 | 81.6893 | −15.3168 | BLLAC | 0.200 | - | 1 | 4 |
| J0527.3−6223 | 81.9394 | −62.4212 | BLLAC | 0.084 | 0.043 | 5 | 5,6,12a,12b,13 |
| J0528.7−5920 | 82.1919 | −59.3344 | BLLAC | 0.124 | 0.031 | 2 | 2,13 |
| J0529.1+0935 | 82.2607 | 9.5765 | UNCL | 0.240 | 0.080 | 2 | 4,6 |
| J0529.1−0101 | 82.2676 | −0.9597 | UNCL | 0.784 | 0.298 | 4 | 1,3,4,6 |
| J0529.3−7243 | 82.3752 | −72.7579 | UNCL | - | - | - | |
| J0529.4−0521 | 82.4731 | −5.3282 | FSRQ | 0.683 | 0.360 | 3 | 1,3,6 |
| J0530.9+1332 | 82.7351 | 13.5320 | FSRQ | 1.140 | 1.181 | 2 | 3,6 |
| J0532.0−4827 | 82.9942 | −48.4600 | BLLAC | 1.134 | 0.797 | 3 | 2,6,13 |
| J0532.6+0732 | 83.1625 | 7.5454 | FSRQ | 1.507 | - | 1 | 3 |
| J0532.8−3941 | 83.2383 | −39.6858 | UNCL | 0.586 | 0.143 | 4 | 6,12a,12b,13 |
| J0532.9−8325 | 83.4098 | −83.4099 | FSRQ | - | - | - | |
| J0533.0−8446 | 83.0139 | −84.7994 | UNCL | - | - | - | |
| J0533.1−6119 | 83.7155 | −61.3657 | UNCL | 1.044 | 0.008 | 2 | 12a,13 |
| J0533.3−5549 | 83.3516 | −55.8268 | UNCL | 0.841 | - | 1 | 13 |
| J0533.8−3749 | 83.5729 | −37.7904 | FSRQ | 0.807 | 0.143 | 2 | 2,13 |
| J0536.0−2754 | 83.9648 | −27.8657 | UNCL | 1.298 | 0.734 | 4 | 2,3,6,13 |
| J0536.4−3343 | 84.1211 | −33.7174 | BLLAC | 0.194 | 0.141 | 2 | 2,13 |
| J0536.4−3401 | 84.1185 | −34.0199 | FSRQ | 0.205 | - | 1 | 13 |
| J0536.5−2548 | 84.1120 | −25.7967 | UNCL | 0.619 | 0.256 | 3 | 2,3,13 |
| J0537.7−5717 | 84.4540 | −57.3084 | BLLAC | 0.131 | 0.026 | 2 | 2,13 |
| J0538.2−3910 | 84.5432 | −39.1451 | BLLAC | 0.211 | 0.058 | 5 | 4,6,12a,12b,13 |
| J0538.6+0443 | 84.6950 | 4.7049 | UNCL | 1.124 | - | 1 | 3 |
| J0538.8−4405 | 84.7098 | −44.0858 | BLLAC | 0.439 | 0.482 | 2 | 2,13 |
| J0539.7−0521c | 84.9997 | −5.2448 | UNCL | 1.835 | 0.047 | 2 | 3,4 |
| J0539.9−2839 | 84.9762 | −28.6655 | FSRQ | 1.128 | 0.604 | 3 | 2,3,13 |
| J0540.5+5823 | 85.1250 | 58.3940 | BLLAC | - | - | - | |
| J0540.8−5415 | 85.1910 | −54.3061 | FSRQ | 0.487 | 0.479 | 3 | 2,6,13 |
| J0541.1−4854 | 85.2754 | −48.9022 | UNCL | - | - | - | |
| J0541.4−7334 | 85.4616 | −73.5376 | UNCL | - | - | - | |
| J0541.6−0541 | 85.4087 | −5.6971 | FSRQ | 0.865 | - | 1 | 3 |
| J0542.8−3458 | 85.7263 | −34.9985 | UNCL | 0.201 | 0.016 | 4 | 4,6,12b,13 |
| J0542.9−0913 | 85.7328 | −9.2253 | UNCL | - | - | - | |
| J0543.9−5531 | 85.9884 | −55.5354 | BLLAC | 0.218 | 0.224 | 4 | 2,6,12a,13 |
| J0545.0+0613c | 86.3714 | 6.3325 | UNCL | 1.370 | 0.360 | 2 | 3,4 |
| J0546.9−2206 | 86.7366 | −22.0826 | BLLAC | 0.213 | 0.031 | 5 | 6,11,12a,12b,13 |
| J0548.5−5218 | 87.1257 | −52.3078 | UNCL | 0.283 | 0.104 | 3 | 2,4,13 |
| J0550.3−5733 | 87.5399 | −57.5401 | FSRQ | 0.520 | 0.161 | 2 | 2,13 |
| J0550.5−3216 | 87.6690 | −32.2712 | BLLAC | 0.055 | 0.004 | 4 | 5,6,12a,13 |
| J0551.0−1622 | 87.7136 | −16.3639 | UNCL | 0.957 | 0.476 | 2 | 3,4 |
| J0551.8−3517 | 87.9263 | −35.2592 | UNCL | 0.332 | 0.204 | 3 | 2,4,13 |
| J0552.8+0313 | 88.2088 | 3.2242 | UNCL | 0.605 | - | 1 | 7 |
| J0553.5−2034 | 88.3880 | −20.5719 | UNCL | 1.070 | 1.265 | 2 | 3,13 |
| J0554.3−1009c | 88.8845 | −10.0353 | UNCL | 1.924 | - | 1 | 3 |
| J0555.1+0304 | 88.7541 | 3.0737 | UNCL | - | - | - | |
| J0556.2−4352 | 89.0781 | −43.8628 | BLLAC | 0.467 | 0.023 | 2 | 2,13 |
| J0557.3−0615 | 89.3201 | −6.2852 | UNCL | 1.107 | 1.077 | 2 | 3,4 |
| J0557.6−0721 | 89.4057 | −7.3205 | UNCL | 0.718 | - | 1 | 3 |
| J0558.0−3837 | 89.5268 | −38.6421 | BLLAC | 1.637 | 2.086 | 2 | 2,13 |
| J0558.1−2859 | 89.4996 | −28.9304 | UNCL | 0.557 | 0.117 | 6 | 3,4,6,12a,12b,13 |
| J0558.8−7459 | 89.6918 | −74.9848 | BLLAC | 0.194 | - | 1 | 6 |
| J0559.9+6409 | 89.9970 | 64.1662 | UNCL | 0.318 | 0.109 | 4 | 1,4,6,11 |
| J0600.6−3939 | 90.1309 | −39.6173 | FSRQ | 0.521 | 0.239 | 2 | 2,13 |
| J0601.1−7035 | 90.2969 | −70.6024 | FSRQ | - | - | - | |
| J0601.3+5444 | 90.2571 | 54.7267 | UNCL | 0.052 | 0.011 | 3 | 5,6,11 |
| J0601.3−7238 | 90.4222 | −72.6426 | UNCL | 0.135 | 0.014 | 2 | 5,6 |
| J0601.8−2003 | 90.4701 | −20.0792 | FSRQ | 1.133 | - | 1 | 3 |
| J0602.0+5315 | 90.5019 | 53.2667 | BLLAC | 0.047 | 0.004 | 3 | 5,6,11 |
| J0602.7−0007 | 90.6787 | −0.0743 | BLLAC | 0.072 | 0.037 | 5 | 5,6,7,8,11 |
| J0602.8−4019 | 90.7137 | −40.3126 | UNCL | 0.204 | 0.129 | 2 | 2,13 |
| J0604.1−4816 | 91.0359 | −48.2903 | BLLAC | 0.130 | - | 1 | 13 |
| J0604.5−4851 | 91.1379 | −48.8299 | UNCL | 0.760 | 0.376 | 3 | 2,6,13 |
| J0604.8+4411 | 91.1485 | 44.2329 | FSRQ | 1.398 | - | 1 | 3 |
| J0604.9−0000 | 91.2434 | 0.0120 | UNCL | - | - | - | |
| J0606.5−4730 | 91.6489 | −47.4986 | SEY | 0.023 | 0.005 | 4 | 5,6,12b,13 |
| J0606.9+4402 | 91.7092 | 44.0280 | UNCL | 0.682 | 0.376 | 2 | 3,4 |
| J0607.2−2518 | 91.8096 | −25.3161 | BLLAC | 0.190 | - | 1 | 6 |
| J0607.4+4739 | 91.8469 | 47.6630 | BLLAC | 1.022 | - | 1 | 3 |
| J0608.0+6721 | 91.9695 | 67.3487 | FSRQ | 1.064 | 0.306 | 2 | 3,13 |
| J0608.0−0835 | 91.9987 | −8.5805 | FSRQ | - | - | - | |
| J0608.1−1521 | 92.0064 | −15.3436 | FSRQ | 0.831 | 0.491 | 2 | 3,6 |
| J0608.1−6028 | 91.9795 | −60.5311 | FSRQ | 0.814 | 0.477 | 3 | 2,4,13 |
| J0608.9−5456 | 92.2044 | −54.9452 | UNCL | 1.004 | 0.860 | 3 | 2,4,13 |
| J0609.0−2219 | 92.2487 | −22.3392 | FSRQ | 1.493 | - | 1 | 3 |
| J0609.2−0247 | 92.3128 | −2.7985 | BLLAC | 0.711 | 0.681 | 2 | 3,4 |
| J0610.1−1848 | 92.5745 | −18.7945 | BLLAC | 0.485 | 0.378 | 2 | 3,6 |
| J0610.9−6054 | 92.6262 | −60.9772 | FSRQ | 1.034 | 0.955 | 2 | 2,13 |
| J0611.1+4325 | 92.7854 | 43.4084 | UNCL | - | - | - | |
| J0611.6−2712 | 92.9426 | −27.1564 | UNCL | 1.063 | 0.351 | 2 | 3,4 |
| J0612.5−3138 | 93.1236 | −31.6495 | FSRQ | 0.436 | - | 1 | 6 |
| J0612.5−3934 | 93.1575 | −39.6498 | UNCL | 0.403 | 0.131 | 4 | 2,4,6,13 |
| J0612.8+4122 | 93.2133 | 41.3771 | BLLAC | 0.764 | 0.894 | 2 | 3,6 |
| J0614.8+6136 | 93.6757 | 61.6523 | UNCL | 0.812 | 0.855 | 3 | 3,4,6 |
| J0615.3−3117 | 93.8300 | −31.2893 | BLLAC | 0.289 | - | 1 | 6 |
| J0616.1−1732 | 94.0429 | −17.5515 | UNCL | - | - | - | |
| J0616.7−1049 | 94.1742 | −10.6857 | UNCL | 1.085 | 0.153 | 2 | 3,4 |
| J0616.9+4340 | 94.2614 | 43.6759 | UNCL | 0.300 | - | 1 | 4 |
| J0617.2+5701 | 94.3205 | 57.0212 | BLLAC | 0.592 | 0.638 | 2 | 3,13 |
| J0617.7−1715 | 94.3892 | −17.2570 | BLLAC | 0.076 | 0.022 | 3 | 5,6,11 |
| J0618.1−2428 | 94.5944 | −24.4439 | FSRQ | 0.278 | 0.119 | 4 | 3,4,6,11 |
| J0618.9−1138 | 94.7671 | −11.6819 | UNCL | 1.286 | - | 1 | 3 |
| J0620.5−2512 | 95.1338 | −25.2549 | FSRQ | 1.714 | 0.248 | 2 | 3,4 |
| J0621.2−2213 | 95.2926 | −22.2285 | UNCL | - | - | - | |
| J0621.2−4648 | 95.3310 | −46.8329 | FSRQ | 0.286 | 0.115 | 2 | 2,13 |
| J0621.7−3411 | 95.4567 | −34.1969 | BLLAC | - | - | - | |
| J0622.3−2605 | 95.5919 | −26.0957 | BLLAC | 0.882 | - | 1 | 3 |
| J0622.4−6433 | 95.7821 | −64.6058 | FSRQ | 0.085 | 0.012 | 2 | 5,6 |
| J0622.7−4141 | 95.6771 | −41.7330 | UNCL | - | - | - | |
| J0623.0−3010 | 95.7981 | −30.1645 | UNCL | - | - | - | |
| J0623.7−3348 | 95.9163 | −33.8374 | UNCL | - | - | - | |
| J0623.9−5259 | 95.9079 | −52.9661 | BLLAC | 0.180 | - | 1 | 13 |
| J0624.2−2943 | 96.0929 | −29.7469 | UNCL | - | - | - | |
| J0625.3+4439 | 96.3261 | 44.6671 | BLLAC | 0.591 | 0.698 | 2 | 3,13 |
| J0625.8−5441 | 96.4676 | −54.6474 | FSRQ | 0.812 | 0.877 | 3 | 2,6,13 |
| J0626.4−1712 | 96.6095 | −17.1796 | UNCL | 0.775 | 0.101 | 2 | 3,4 |
| J0626.4−4259 | 96.6529 | −42.9683 | UNCL | 0.300 | - | 1 | 4 |
| J0627.0−3529 | 96.7780 | −35.4876 | MIS | 0.022 | 0.012 | 2 | 5,6 |
| J0628.6+6900 | 97.3427 | 69.0054 | UNCL | 0.131 | 0.051 | 5 | 3,4,6,11,13 |
| J0628.8−6250 | 97.2395 | −62.8124 | BLLAC | - | - | - | |
| J0629.3−1959 | 97.3490 | −19.9888 | BLLAC | 1.293 | - | 1 | 3 |
| J0630.2+3228 | 97.5445 | 32.4361 | UNCL | 0.717 | - | 1 | 11 |
| J0630.9−2406 | 97.7480 | −24.1128 | BLLAC | 1.229 | - | 1 | 3 |
| J0633.4−2222 | 98.3615 | −22.3895 | FSRQ | 2.434 | - | 1 | 3 |
| J0634.9−2335 | 98.7458 | −23.5867 | FSRQ | 1.114 | - | 1 | 3 |
| J0635.6−7518 | 98.9438 | −75.2713 | FSRQ | - | - | - | |
| J0636.5+7138 | 99.1787 | 71.6454 | UNCL | 1.169 | - | 1 | 3 |
| J0637.4−3537 | 99.4434 | −35.6134 | UNCL | 0.478 | 0.029 | 2 | 4,6 |
| J0638.2+6020 | 99.6490 | 60.2842 | UNCL | 0.386 | 0.214 | 3 | 3,4,13 |
| J0638.6+7320 | 99.8415 | 73.4161 | FSRQ | 1.778 | - | 1 | 3 |
| J0638.7+5658 | 99.6073 | 57.0307 | UNCL | 0.704 | 0.395 | 3 | 3,4,13 |
| J0639.6+3503 | 99.7900 | 35.1063 | UNCL | 0.772 | 0.523 | 4 | 3,4,6,13 |
| J0643.2−5356 | 100.8342 | −53.9797 | UNCL | 0.300 | - | 1 | 4 |
| J0644.4−6712 | 101.1169 | −67.2159 | FSRQ | 0.550 | - | 1 | 6 |
| J0644.6+6039 | 101.1489 | 60.6475 | BLLAC | 0.234 | 0.088 | 2 | 4,13 |
| J0644.6−2853 | 101.1823 | −28.8546 | BLLAC | 0.784 | 0.512 | 2 | 3,4 |
| J0646.7−3913 | 101.6288 | −39.0609 | FSRQ | - | - | - | |
| J0647.0−5138 | 101.7918 | −51.5966 | BLLAC | 0.161 | 0.053 | 2 | 4,6 |
| J0647.7−4418 | 101.9463 | −44.3306 | UNCL | - | - | - | |
| J0647.7−6058 | 101.9202 | −60.9681 | BLLAC | - | - | - | |
| J0647.8+4527 | 101.9580 | 45.4197 | UNCL | 0.577 | 0.450 | 2 | 3,13 |
| J0648.0−3045 | 102.0587 | −30.7388 | FSRQ | - | - | - | |
| J0648.4−6941 | 102.2104 | −69.7563 | BLLAC | 0.266 | 0.045 | 2 | 4,6 |
| J0649.5−3139 | 102.3900 | −31.6556 | UNCL | - | - | - | |
| J0650.5−2851 | 102.6372 | −28.8216 | UNCL | - | - | - | |
| J0650.7+2503 | 102.6937 | 25.0499 | BLLAC | - | - | - | |
| J0651.0+4013 | 102.7726 | 40.2272 | BLLAC | 0.316 | 0.287 | 4 | 3,4,6,13 |
| J0651.4+6525 | 102.8555 | 65.4158 | UNCL | 0.600 | 0.299 | 4 | 1,3,4,13 |
| J0651.5+7956 | 102.9949 | 79.9422 | UNCL | 0.793 | 0.718 | 4 | 3,4,12b,13 |
| J0652.1−4813 | 103.0024 | −48.1498 | BLLAC | 0.400 | - | 1 | 4 |
| J0653.7+2815 | 103.4345 | 28.2631 | BLLAC | 0.891 | - | 1 | 3 |
| J0654.0−4152 | 103.4995 | −41.8625 | MIS | 0.086 | 0.015 | 2 | 5,6 |
| J0654.3+5042 | 103.5921 | 50.7066 | FSRQ | 0.019 | - | 1 | 13 |
| J0654.4+4514 | 103.5988 | 45.2399 | FSRQ | 0.808 | 0.579 | 2 | 3,13 |
| J0654.6−4952 | 103.8268 | −49.8683 | UNCL | - | - | - | |
| J0654.7+4246 | 103.6814 | 42.7996 | BLLAC | 0.079 | 0.021 | 5 | 5,6,11,12b,13 |
| J0656.3+4235 | 104.0444 | 42.6174 | BLLAC | 0.047 | 0.013 | 5 | 5,6,11,12b,13 |
| J0658.1−5840 | 104.5574 | −58.6743 | FSRQ | - | - | - | |
| J0658.2+2709 | 104.5386 | 27.1396 | UNCL | 1.210 | - | 1 | 3 |
| J0659.6−2742 | 104.9580 | −27.7551 | FSRQ | 1.728 | - | 1 | 3 |
| J0659.6−6742 | 104.8872 | −67.7306 | UNCL | 0.424 | 0.033 | 2 | 4,6 |
| J0700.1−6311 | 104.9945 | −63.2108 | UNCL | 0.592 | 0.011 | 2 | 4,6 |
| J0700.5−6610 | 105.1302 | −66.1792 | BLLAC | - | - | - | |
| J0701.5+2511 | 105.3840 | 25.1649 | UNCL | 0.602 | 0.622 | 3 | 3,4,6 |
| J0701.5−4634 | 105.3939 | −46.5768 | FSRQ | - | - | - | |
| J0703.2−3914 | 105.8027 | −39.2386 | UNCL | - | - | - | |
| J0704.7+4508 | 106.2124 | 45.0449 | UNCL | 0.613 | 0.357 | 3 | 3,4,13 |
| J0704.8+4907 | 106.2497 | 49.1101 | UNCL | 0.619 | 0.054 | 2 | 12b,13 |
| J0705.7−4848 | 106.4947 | −48.7901 | UNCL | - | - | - | |
| J0705.9+5309 | 106.5306 | 53.1653 | UNCL | 0.626 | 0.318 | 5 | 3,4,6,12b,13 |
| J0706.5+3744 | 106.6321 | 37.7434 | BLLAC | 0.656 | 0.804 | 2 | 3,13 |
| J0706.8+7742 | 106.7139 | 77.6936 | BLLAC | 0.566 | 0.652 | 2 | 3,13 |
| J0706.9+6109 | 106.7526 | 61.1699 | BLLAC | 0.327 | 0.268 | 3 | 3,6,13 |
| J0708.9+4839 | 107.2834 | 48.6155 | MIS | 0.013 | 0.003 | 4 | 5,6,11,13 |
| J0709.1+2241 | 107.2429 | 22.6932 | BLLAC | 0.331 | 0.256 | 2 | 3,6 |
| J0710.4+5908 | 107.6253 | 59.1390 | BLLAC | 0.084 | 0.025 | 4 | 5,6,11,13 |
| J0710.8−3851 | 107.6818 | −38.8436 | FSRQ | 0.108 | 0.001 | 2 | 5,6 |
| J0710.9+4733 | 107.6921 | 47.5364 | FSRQ | 0.078 | - | 1 | 13 |
| J0712.4+5724 | 108.0788 | 57.3301 | BLLAC | 0.436 | 0.151 | 3 | 6,12b,13 |
| J0712.7+5033 | 108.1820 | 50.5563 | BLLAC | 0.460 | 0.464 | 2 | 3,13 |
| J0713.0+5738 | 108.2689 | 57.6361 | UNCL | 0.600 | 0.502 | 3 | 3,4,13 |
| J0713.5+2537 | 108.4030 | 25.6714 | UNCL | - | - | - | |
| J0713.8+1935 | 108.4820 | 19.5834 | FSRQ | 1.351 | - | 1 | 3 |
| J0714.4+1110 | 108.5691 | 11.1417 | UNCL | 1.004 | 0.273 | 2 | 3,4 |
| J0715.3−6828 | 108.7896 | −68.4995 | UNCL | - | - | - | |
| J0715.6−4528 | 108.9363 | −45.5085 | UNCL | 0.175 | - | 1 | 6 |
| J0717.7−5519 | 109.4378 | −55.3394 | UNCL | - | - | - | |
| J0718.0+4536 | 109.4661 | 45.6342 | FSRQ | 0.623 | 0.777 | 2 | 3,13 |
| J0718.6−4319 | 109.6818 | −43.3305 | BLLAC | - | - | - | |
| J0719.1−7055 | 109.7859 | −70.9010 | BLLAC | 0.184 | - | 1 | 6 |
| J0719.3+3307 | 109.8309 | 33.1194 | CLAGN | 0.699 | 0.842 | 2 | 3,13 |
| J0719.7−4012 | 109.9133 | −40.1965 | BLLAC | 0.223 | - | 1 | 6 |
| J0720.0−6237 | 109.7686 | −62.3007 | FSRQ | - | - | - | |
| J0721.9+7120 | 110.4727 | 71.3434 | BLLAC | 0.033 | - | 1 | 13 |
| J0722.7+3606 | 110.7392 | 36.1055 | UNCL | 0.786 | 0.296 | 5 | 1,3,4,6,13 |
| J0723.4+5841 | 110.8086 | 58.6891 | UNCL | 0.232 | 0.043 | 4 | 4,6,12b,13 |
| J0723.5+2900 | 110.9785 | 28.9916 | FSRQ | 0.554 | 0.419 | 3 | 3,6,13 |
| J0723.7+2050 | 110.9514 | 20.8585 | BLLAC | 0.555 | 0.588 | 3 | 3,4,13 |
| J0725.2+1425 | 111.3200 | 14.4205 | FSRQ | 0.722 | 0.367 | 3 | 1,3,6 |
| J0726.1+8114 | 111.3596 | 81.2355 | UNCL | 0.120 | 0.005 | 2 | 11,13 |
| J0726.4−4727 | 111.6093 | −47.4815 | FSRQ | 0.317 | - | 1 | 6 |
| J0727.1+3734 | 111.7480 | 37.5731 | BLLAC | 0.456 | - | 2 | 1,13 |
| J0728.0+6735 | 112.2236 | 67.5410 | UNCL | 0.963 | 0.004 | 2 | 12b,13 |
| J0728.2+4827 | 111.9994 | 48.4557 | BLLAC | 0.187 | 0.080 | 3 | 3,6,13 |
| J0728.5+6128 | 112.3457 | 61.4867 | UNCL | 0.745 | 0.290 | 4 | 3,4,6,13 |
| J0729.1+5703 | 112.2068 | 57.0234 | FSRQ | 0.268 | 0.232 | 3 | 3,6,13 |
| J0730.4+3308 | 112.6086 | 33.1230 | BLLAC | 0.453 | 0.440 | 2 | 3,13 |
| J0730.7−6602 | 112.7065 | −66.0386 | BLLAC | 0.068 | 0.008 | 2 | 5,6 |
| J0731.9+2805 | 112.9697 | 28.0758 | BLLAC | 0.161 | 0.041 | 7 | 5,6,7,8,11,12b,13 |
| J0732.7−4638 | 113.1846 | −46.6714 | UNCL | 0.457 | - | 1 | 6 |
| J0733.0+4915 | 113.2433 | 49.2826 | UNCL | 0.668 | 0.179 | 3 | 3,4,13 |
| J0733.1+5910 | 113.2739 | 59.1483 | UNCL | 0.756 | 0.012 | 3 | 11,12b,13 |
| J0733.4+5152 | 113.3616 | 51.8989 | BLLAC | 0.066 | 0.020 | 4 | 4,11,12b,13 |
| J0733.5−5445 | 113.3948 | −54.7616 | UNCL | - | - | - | |
| J0733.6+3649 | 113.3516 | 36.8346 | BLLAC | 0.343 | - | 1 | 13 |
| J0733.7+0205c | 113.4783 | 2.0395 | UNCL | - | - | - | |
| J0733.7+4110 | 113.4450 | 41.1889 | AMB | 0.599 | 0.482 | 3 | 1,3,13 |
| J0733.8+0455 | 113.4894 | 4.9374 | FSRQ | - | - | - | |
| J0734.0+5021 | 113.4688 | 50.3692 | FSRQ | 0.430 | 0.558 | 2 | 3,13 |
| J0734.4−7711 | 113.6809 | −77.1871 | UNCL | - | - | - | |
| J0737.3−8247 | 114.2754 | −82.8111 | UNCL | 0.200 | - | 1 | 4 |
| J0738.1+1742 | 114.5308 | 17.7053 | BLLAC | 0.299 | 0.207 | 2 | 3,13 |
| J0738.4+1539 | 114.6040 | 15.6444 | UNCL | - | - | - | |
| J0739.2+0137 | 114.8251 | 1.6179 | FSRQ | 0.399 | 0.326 | 2 | 3,6 |
| J0739.8−6722 | 114.8640 | −67.3602 | UNCL | 0.500 | - | 1 | 4 |
| J0740.9+3203 | 115.2748 | 32.0956 | BLLAC | 0.146 | 0.022 | 8 | 5,6,7,8,10,11,12b,13 |
| J0741.0+3226 | 115.2275 | 32.4336 | BLLAC | 0.614 | 0.368 | 3 | 1,3,13 |
| J0741.2−5140 | 115.2103 | −51.6255 | UNCL | - | - | - | |
| J0741.4−4709 | 115.4385 | −47.1572 | FSRQ | - | - | - | |
| J0742.1+4902 | 115.5115 | 49.0043 | FSRQ | 0.965 | 0.291 | 4 | 1,3,6,13 |
| J0742.6+5443 | 115.6658 | 54.7402 | FSRQ | 0.451 | 0.106 | 3 | 3,6,13 |
| J0742.9−5242 | 115.6863 | −52.6852 | UNCL | - | - | - | |
| J0743.0−5622 | 115.8354 | −56.3258 | FSRQ | - | - | - | |
| J0743.1+1713 | 115.7713 | 17.2401 | BLLAC | 0.579 | 0.244 | 3 | 1,3,13 |
| J0743.3−4912c | 115.7690 | −49.1703 | UNCL | - | - | - | |
| J0744.1+7434 | 116.0224 | 74.5662 | BLLAC | 0.046 | - | 1 | 13 |
| J0744.2−6918 | 116.0850 | −69.3187 | BLLAC | - | - | - | |
| J0746.0−0039 | 116.4753 | −0.7382 | FSRQ | 2.278 | - | 1 | 3 |
| J0746.3−0225 | 116.6126 | −2.4304 | UNCL | 0.622 | 0.509 | 2 | 3,6 |
| J0746.4+2546 | 116.6078 | 25.8173 | FSRQ | 1.544 | 1.074 | 3 | 1,3,13 |
| J0746.5+2730 | 116.6685 | 27.5831 | BLLAC | 0.793 | 0.243 | 3 | 1,3,13 |
| J0746.6−4754 | 116.6763 | −47.9154 | BLLAC | - | - | - | |
| J0747.5+0905 | 116.8425 | 9.0968 | BLLAC | 0.194 | 0.075 | 3 | 4,6,13 |
| J0747.5−4927 | 116.8531 | −49.4425 | UNCL | 0.405 | - | 1 | 6 |
| J0748.3+4928 | 117.1574 | 49.5114 | BLLAC | 0.748 | 0.855 | 6 | 3,4,7,8,11,13 |
| J0748.3+8511 | 116.8173 | 85.2024 | UNCL | 0.246 | 0.072 | 2 | 4,6 |
| J0748.6+2400 | 117.1505 | 24.0067 | FSRQ | 0.441 | 0.282 | 3 | 1,3,13 |
| J0749.2+2314 | 117.3085 | 23.2214 | BLLAC | 0.154 | 0.026 | 8 | 5,6,7,8,10,11,12b,13 |
| J0749.3+4453 | 117.3204 | 44.8756 | FSRQ | 0.618 | 0.433 | 4 | 3,7,8,13 |
| J0749.4+1058 | 117.3641 | 10.9592 | BLLAC | 0.463 | 0.425 | 2 | 3,13 |
| J0749.6+1324 | 117.3998 | 13.3656 | UNCL | 0.859 | 0.311 | 5 | 1,3,4,6,13 |
| J0749.7+7450 | 117.3732 | 74.8624 | BLLAC | 0.168 | 0.044 | 2 | 6,13 |
| J0749.9+1823 | 117.5014 | 18.3865 | FSRQ | 0.764 | 0.300 | 3 | 1,3,13 |
| J0750.8+1229 | 117.7169 | 12.5180 | FSRQ | 0.384 | 0.392 | 3 | 3,6,13 |
| J0751.0+7908 | 117.6803 | 79.1547 | UNCL | 0.543 | 0.295 | 3 | 3,11,13 |
| J0751.0−5131 | 117.7491 | −51.5790 | UNCL | 0.275 | - | 1 | 6 |
| J0751.4+2655 | 117.9047 | 26.9522 | BLLAC | 0.699 | 0.342 | 3 | 1,3,13 |
| J0751.4−0421 | 117.8446 | −4.3607 | UNCL | 0.269 | - | 1 | 11 |
| J0752.2+3313 | 117.9736 | 33.2222 | FSRQ | 1.352 | 0.833 | 3 | 1,3,13 |
| J0753.0+5353 | 118.2558 | 53.8832 | BLLAC | 0.270 | 0.168 | 3 | 3,4,13 |
| J0753.9+0923 | 118.4664 | 9.4055 | UNCL | 0.923 | 0.010 | 2 | 12b,13 |
| J0754.0+0451 | 118.5238 | 4.8774 | UNCL | 0.733 | - | 1 | 11 |
| J0754.7+4823 | 118.6903 | 48.3974 | BLLAC | 0.737 | 0.825 | 2 | 3,13 |
| J0756.3−6431 | 119.1025 | −64.5085 | UNCL | 0.296 | - | 1 | 6 |
| J0757.1+0956 | 119.2777 | 9.9430 | BLLAC | 0.637 | 0.704 | 2 | 3,13 |
| J0758.1+1134 | 119.5319 | 11.6128 | FSRQ | 0.429 | 0.225 | 3 | 1,3,13 |
| J0758.7+3746 | 119.6171 | 37.7866 | MIS | 0.034 | 0.022 | 7 | 5,6,7,8,10,12b,13 |
| J0758.9+2703 | 119.6958 | 27.0877 | BLLAC | 0.112 | 0.021 | 5 | 5,6,7,8,13 |
| J0759.6+1321 | 119.9006 | 13.3549 | BLLAC | 0.693 | 0.822 | 3 | 3,6,13 |
| J0800.3+5611 | 120.0647 | 56.1854 | UNCL | 0.621 | 0.289 | 4 | 3,4,6,13 |
| J0800.9+4401 | 120.2845 | 44.0195 | BLLAC | 0.682 | 0.300 | 3 | 1,3,13 |
| J0801.1+1335 | 120.3127 | 13.6118 | BLLAC | 0.686 | 0.305 | 2 | 1,13 |
| J0801.1+6444 | 120.2594 | 64.7471 | BLLAC | 0.188 | 0.035 | 3 | 4,6,13 |
| J0801.3+6631 | 120.4016 | 66.6528 | UNCL | 0.681 | 0.393 | 4 | 1,3,4,13 |
| J0802.0+1006 | 120.4975 | 10.0934 | BLLAC | - | - | - | |
| J0802.3−0942 | 120.5653 | −9.7139 | UNCL | - | - | - | |
| J0803.0+2439 | 120.7804 | 24.6308 | BLLAC | 0.722 | 0.475 | 3 | 1,3,13 |
| J0803.2−0337 | 120.8003 | −3.6002 | UNCL | 0.542 | 0.431 | 2 | 3,6 |
| J0803.5+2046 | 120.7778 | 20.6415 | FSRQ | 1.442 | 0.775 | 3 | 1,3,13 |
| J0804.5+0414 | 121.1813 | 4.2361 | UNCL | 0.482 | 0.200 | 3 | 3,4,13 |
| J0804.9−0624 | 121.2406 | −6.4073 | UNCL | 0.300 | - | 1 | 4 |
| J0805.0+6746 | 121.2573 | 67.7670 | UNCL | 0.740 | 0.244 | 3 | 3,4,13 |
| J0805.1+7744 | 121.6559 | 77.7687 | UNCL | 1.573 | 0.383 | 3 | 3,4,13 |
| J0805.2−0110 | 121.3037 | −1.1872 | FSRQ | 0.969 | 0.659 | 3 | 3,6,13 |
| J0805.4+6147 | 121.3257 | 61.7399 | FSRQ | 1.250 | 0.595 | 2 | 3,13 |
| J0805.4+7534 | 121.3610 | 75.5736 | BLLAC | 0.088 | 0.011 | 3 | 5,6,13 |
| J0805.9+3834 | 121.4657 | 38.5939 | BLLAC | 0.576 | 0.151 | 3 | 1,3,13 |
| J0806.1−0458 | 121.5366 | −4.9032 | UNCL | 0.865 | 0.354 | 2 | 3,4 |
| J0806.5+4503 | 121.6395 | 45.0756 | FSRQ | 1.181 | 0.489 | 3 | 1,3,13 |
| J0806.5+5930 | 121.6081 | 59.5186 | BLLAC | 0.159 | 0.073 | 5 | 4,5,6,11,13 |
| J0807.0−6102 | 121.7054 | −61.0250 | UNCL | - | - | - | |
| J0807.1−0541 | 121.7901 | −5.6872 | BLLAC | 0.837 | - | 1 | 3 |
| J0807.2−7630 | 121.8752 | −76.4866 | UNCL | 0.481 | - | 1 | 6 |
| J0807.7−1206 | 121.9000 | −12.1288 | UNCL | 1.105 | 0.141 | 2 | 3,4 |
| J0808.2−0751 | 122.0647 | −7.8527 | FSRQ | 1.068 | - | 1 | 3 |
| J0808.5+4950 | 122.1653 | 49.8435 | FSRQ | 1.190 | 1.427 | 2 | 3,13 |
| J0809.3+4053 | 122.2361 | 40.8791 | FSRQ | 0.750 | 0.579 | 4 | 1,3,6,13 |
| J0809.5+5341 | 122.4239 | 53.6903 | FSRQ | 0.803 | 0.298 | 3 | 1,3,13 |
| J0809.6+3455 | 122.4120 | 34.9270 | BLLAC | 0.068 | 0.010 | 8 | 5,6,7,8,10,11,12b,13 |
| J0809.8+5218 | 122.4549 | 52.3162 | BLLAC | 0.055 | 0.026 | 2 | 6,13 |
| J0811.0−7529 | 122.7634 | −75.5077 | BLLAC | - | - | - | |
| J0811.4+0146 | 122.8613 | 1.7812 | BLLAC | 0.579 | 0.550 | 3 | 1,3,13 |
| J0812.0+0237 | 123.0077 | 2.6259 | BLLAC | 0.130 | 0.035 | 6 | 5,6,7,8,12b,13 |
| J0812.3+1143 | 123.1084 | 11.6996 | BLLAC | 0.463 | 0.064 | 4 | 1,3,6,13 |
| J0812.5+0711 | 123.1576 | 7.2002 | UNCL | 0.908 | 0.261 | 4 | 1,3,4,13 |
| J0812.6+2821 | 123.1302 | 28.3490 | BLLAC | 0.909 | 0.770 | 4 | 1,3,6,13 |
| J0812.8+6507 | 123.1702 | 65.1531 | BLLAC | 0.170 | 0.039 | 7 | 4,6,7,8,11,12b,13 |
| J0812.9+5555 | 123.2144 | 55.9060 | BLLAC | 0.288 | 0.086 | 4 | 1,3,6,13 |
| J0813.7−0356 | 123.4086 | −3.9548 | UNCL | 0.256 | 0.058 | 2 | 4,6 |
| J0814.2−1013 | 123.5487 | −10.2029 | BLLAC | 0.767 | 0.860 | 2 | 3,6 |
| J0814.4+2941 | 123.6079 | 29.6877 | FSRQ | 0.454 | 0.182 | 3 | 1,3,13 |
| J0814.4+6926 | 123.5249 | 69.4413 | UNCL | 0.630 | 0.227 | 2 | 4,13 |
| J0814.6+6430 | 123.6633 | 64.5228 | BLLAC | 0.213 | 0.118 | 4 | 3,5,6,13 |
| J0815.6+3641 | 123.8581 | 36.5875 | FSRQ | 0.743 | 0.468 | 3 | 1,3,13 |
| J0815.9+2951 | 123.9019 | 29.8394 | BLLAC | 0.259 | 0.037 | 6 | 6,7,8,11,12b,13 |
| J0816.1+4909 | 124.0399 | 49.1679 | BLLAC | 0.371 | 0.267 | 2 | 3,13 |
| J0816.3+5739 | 124.0947 | 57.6525 | BLLAC | 0.404 | 0.403 | 2 | 3,13 |
| J0816.4−1311 | 124.1133 | −13.1980 | BLLAC | - | - | - | |
| J0816.9+2050 | 124.2074 | 20.8518 | BLLAC | 0.867 | 0.973 | 2 | 3,13 |
| J0817.1+1955 | 124.2729 | 19.9786 | AMB | 0.611 | 0.211 | 3 | 1,3,13 |
| J0817.8+3243 | 124.4625 | 32.7279 | BLLAC | 0.752 | 0.244 | 3 | 1,3,13 |
| J0817.8−0934 | 124.4573 | −9.5585 | BLLAC | 1.024 | - | 1 | 3 |
| J0818.2+4222 | 124.5667 | 42.3793 | BLLAC | 0.610 | 0.683 | 2 | 3,13 |
| J0818.4+2816 | 124.6140 | 28.2341 | BLLAC | 0.176 | 0.149 | 4 | 3,6,11,13 |
| J0818.7+3153 | 124.6669 | 31.8967 | BLLAC | 0.671 | 0.326 | 3 | 1,3,13 |
| J0818.8+3229 | 124.7597 | 32.4437 | FSRQ | 0.787 | 0.161 | 4 | 1,3,12b,13 |
| J0819.0+2746 | 124.8286 | 27.7919 | BLLAC | 0.578 | 0.277 | 3 | 1,3,13 |
| J0819.4+4035 | 124.8579 | 40.6289 | BLLAC | 0.365 | 0.112 | 5 | 1,3,6,12b,13 |
| J0819.4−0756 | 124.8233 | −7.9406 | BLLAC | 0.299 | 0.117 | 2 | 3,6 |
| J0820.3+3639 | 125.0841 | 36.6679 | BLLAC | 0.447 | 0.249 | 4 | 1,3,6,13 |
| J0820.9+2353 | 125.2133 | 23.8959 | BLLAC | 0.267 | 0.099 | 5 | 1,3,6,12b,13 |
| J0820.9−1258 | 125.2394 | −12.9831 | BLLAC | 1.094 | - | 1 | 3 |
| J0821.1+1007 | 125.2284 | 10.1026 | FSRQ | 1.282 | 0.568 | 3 | 1,3,13 |
| J0823.1+4042 | 125.7398 | 40.6972 | FSRQ | 0.573 | 0.343 | 3 | 1,3,13 |
| J0823.1−6330 | 125.8108 | −63.4917 | UNCL | 0.202 | 0.011 | 2 | 5,6 |
| J0823.3+2224 | 125.8532 | 22.3842 | BLLAC | 0.719 | 0.503 | 4 | 1,3,6,13 |
| J0824.4+2440 | 126.1375 | 24.6453 | FSRQ | 0.841 | 0.118 | 3 | 1,3,13 |
| J0824.7+5552 | 126.1968 | 55.8785 | FSRQ | 0.970 | 0.559 | 3 | 1,3,13 |
| J0824.9+3915 | 126.2312 | 39.2783 | FSRQ | 0.640 | 0.619 | 2 | 3,13 |
| J0825.8+0309 | 126.4597 | 3.1568 | BLLAC | 0.817 | 0.528 | 3 | 1,3,13 |
| J0826.4−6404 | 126.6161 | −64.0709 | UNCL | 0.204 | 0.006 | 2 | 4,6 |
| J0827.0−0708 | 126.7757 | −7.1461 | BLLAC | 0.120 | 0.028 | 3 | 5,6,13 |
| J0827.8+5221 | 126.9737 | 52.2995 | FSRQ | 0.329 | 0.068 | 6 | 3,6,7,8,12b,13 |
| J0828.0+2307 | 127.0048 | 23.2049 | BLLAC | 0.453 | 0.101 | 3 | 1,6,13 |
| J0828.3+4152 | 127.0592 | 41.8977 | BLLAC | 0.179 | 0.031 | 6 | 6,7,8,11,12b,13 |
| J0828.6−0747 | 127.2270 | −7.8152 | UNCL | 0.415 | 0.003 | 3 | 6,12b,13 |
| J0829.0+1755 | 127.2701 | 17.9044 | MIS | 0.075 | 0.018 | 8 | 5,6,7,8,10,11,12b,13 |
| J0829.4+0857 | 127.3763 | 8.9726 | MIS | 0.601 | 0.249 | 5 | 3,6,7,8,13 |
| J0829.6−1140 | 127.4132 | −11.6843 | UNCL | 0.386 | 0.248 | 2 | 3,4 |
| J0829.7−5856 | 127.3799 | −58.9335 | UNCL | - | - | - | |
| J0830.0+5231 | 127.5455 | 52.5075 | BLLAC | 0.198 | 0.021 | 6 | 6,7,8,11,12b,13 |
| J0830.1−0946 | 127.5631 | −9.7488 | UNCL | 0.500 | - | 1 | 4 |
| J0830.8+2410 | 127.7170 | 24.1833 | FSRQ | 0.584 | 0.738 | 2 | 3,13 |
| J0831.4+2631 | 127.8264 | 26.5070 | UNCL | 1.046 | 0.405 | 2 | 3,13 |
| J0831.5+1747 | 127.8877 | 17.7752 | BLLAC | 0.539 | 0.485 | 5 | 1,3,4,6,13 |
| J0831.8+0429 | 127.9537 | 4.4942 | BLLAC | 0.196 | 0.121 | 3 | 3,6,13 |
| J0832.2+2753 | 128.0819 | 27.8789 | UNCL | 0.255 | 0.289 | 2 | 6,13 |
| J0832.4+4912 | 128.0967 | 49.2225 | BLLAC | 0.330 | 0.219 | 4 | 1,3,6,13 |
| J0833.4−0458 | 128.3270 | −4.9165 | FSRQ | 2.212 | 1.511 | 3 | 1,3,13 |
| J0833.9+4223 | 128.4745 | 42.4005 | CLAGN | 0.941 | 1.084 | 2 | 3,13 |
| J0834.6+4402 | 128.7425 | 44.0606 | BLLAC | 0.518 | 0.552 | 2 | 3,13 |
| J0835.0+6243 | 128.7258 | 62.8302 | UNCL | 1.635 | 1.020 | 2 | 4,13 |
| J0835.2−2243 | 128.6842 | −22.6869 | FSRQ | 1.121 | - | 1 | 3 |
| J0835.7+0936 | 128.9301 | 9.6217 | BLLAC | 0.544 | 0.118 | 3 | 1,3,13 |
| J0836.2+2141 | 129.0676 | 21.6510 | UNCL | 0.776 | 0.262 | 4 | 1,3,4,13 |
| J0836.5−2026 | 129.1634 | −20.2832 | FSRQ | 2.497 | - | 1 | 3 |
| J0837.3+1458 | 129.3530 | 14.9722 | BLLAC | 0.152 | 0.080 | 5 | 6,7,8,12b,13 |
| J0839.4+1803 | 129.8780 | 18.0464 | BLLAC | 0.289 | 0.177 | 3 | 3,6,13 |
| J0839.7+3540 | 129.9307 | 35.6671 | BLLAC | 0.546 | 0.418 | 3 | 1,3,13 |
| J0839.8+0105 | 129.9567 | 1.0741 | FSRQ | 0.707 | 0.502 | 4 | 1,3,6,13 |
| J0840.8+1317 | 130.1983 | 13.2065 | MIS | 0.757 | 0.022 | 3 | 1,3,13 |
| J0841.3+7053 | 130.3515 | 70.8950 | FSRQ | 1.085 | 1.376 | 2 | 3,13 |
| J0842.3−6053 | 130.6107 | −60.8973 | UNCL | - | - | - | |
| J0842.5+0251 | 130.6063 | 2.8813 | BLLAC | 0.233 | 0.089 | 7 | 6,7,8,11,12b,12c,13 |
| J0842.7+6656 | 130.6800 | 66.9581 | BLLAC | 0.185 | 0.052 | 4 | 6,11,12b,13 |
| J0843.0−0853 | 130.8888 | −8.8162 | UNCL | 1.214 | 1.048 | 2 | 4,13 |
| J0844.2+5312 | 131.0487 | 53.2141 | BLLAC | 0.360 | 0.197 | 3 | 1,3,13 |
| J0845.4+0442 | 131.3214 | 4.6632 | UNCL | 0.597 | 0.189 | 5 | 1,3,4,6,13 |
| J0846.5−2609 | 131.7359 | −26.1307 | UNCL | - | - | - | |
| J0846.9+4608 | 131.8929 | 46.1578 | FSRQ | 0.835 | 0.567 | 3 | 1,3,13 |
| J0847.0−2336 | 131.7565 | −23.6171 | BLLAC | 0.045 | 0.009 | 3 | 5,6,11 |
| J0847.2+1134 | 131.8039 | 11.5639 | BLLAC | 0.133 | 0.052 | 4 | 6,7,8,13 |
| J0847.9−0702 | 131.9864 | −7.0547 | BLLAC | 0.441 | 0.400 | 2 | 3,13 |
| J0848.0−0524 | 131.9947 | −5.3428 | FSRQ | 0.882 | 0.244 | 2 | 3,13 |
| J0848.7+0508 | 132.1653 | 5.1050 | BLLAC | 0.305 | 0.264 | 2 | 1,13 |
| J0848.7+7017 | 132.1646 | 70.2910 | BLLAC | 0.811 | 0.378 | 2 | 3,13 |
| J0848.9+0205 | 132.2867 | 2.1062 | BLLAC | 0.636 | 0.361 | 4 | 1,3,6,13 |
| J0849.1+6607 | 132.2276 | 66.1026 | BLLAC | 0.094 | - | 1 | 13 |
| J0849.5+0456 | 132.3856 | 4.9188 | BLLAC | 0.531 | 0.540 | 2 | 3,13 |
| J0850.0+4855 | 132.5015 | 48.9163 | BLLAC | 0.442 | 0.287 | 3 | 1,3,13 |
| J0850.0+5108 | 132.4916 | 51.1414 | NLS1 | 0.508 | 0.210 | 4 | 3,5,6,13 |
| J0850.1−1212 | 132.5401 | −12.2265 | FSRQ | 1.320 | - | 1 | 3 |
| J0850.5+3455 | 132.6508 | 34.9230 | BLLAC | 0.101 | 0.023 | 8 | 5,6,7,8,10,11,12b,13 |
| J0851.5+5528 | 132.8997 | 55.4762 | BLLAC | 0.569 | 0.436 | 3 | 1,3,13 |
| J0852.2+2834 | 133.0215 | 28.5666 | FSRQ | 1.138 | 0.553 | 3 | 1,3,13 |
| J0854.0+2753 | 133.5424 | 27.9060 | BLLAC | 0.399 | 0.088 | 6 | 6,7,8,11,12b,13 |
| J0854.3+4408 | 133.5412 | 44.1417 | BLLAC | 0.093 | - | 1 | 13 |
| J0854.8+2006 | 133.7036 | 20.1085 | BLLAC | 0.524 | 0.616 | 2 | 3,13 |
| J0855.4−0714 | 133.7895 | −7.2508 | UNCL | 0.827 | 0.615 | 2 | 3,13 |
| J0855.9+7144 | 134.2286 | 71.7733 | FSRQ | 0.943 | 0.205 | 2 | 3,13 |
| J0856.6−1105 | 134.1742 | −11.0873 | BLLAC | 1.205 | - | 1 | 3 |
| J0856.8+2056 | 134.1656 | 20.9621 | BLLAC | 0.376 | 0.202 | 4 | 1,3,6,13 |
| J0856.8+8559 | 134.4231 | 86.0624 | UNCL | 0.679 | 0.639 | 2 | 3,4 |
| J0857.7+0137 | 134.4575 | 1.5918 | BLLAC | 0.175 | 0.063 | 8 | 3,5,6,7,8,11,12b,13 |
| J0857.9−1949 | 134.5223 | −19.8436 | FSRQ | 0.911 | - | 1 | 3 |
| J0858.1+1405 | 134.6727 | 14.1624 | MIS | 1.008 | 0.225 | 3 | 1,3,13 |
| J0859.4+6218 | 134.8777 | 62.2918 | BLLAC | 0.346 | 0.158 | 3 | 1,3,13 |
| J0859.4+8345 | 134.7920 | 83.7500 | BLLAC | 0.479 | 0.440 | 5 | 1,3,6,12b,13 |
| J0900.6−7408 | 134.9971 | −74.2336 | UNCL | 0.300 | - | 1 | 4 |
| J0900.7−1243 | 135.1657 | −12.7091 | UNCL | 0.479 | 0.172 | 3 | 3,4,6 |
| J0901.2+6742 | 135.1611 | 67.7065 | BLLAC | 0.970 | 0.512 | 3 | 3,6,13 |
| J0901.4+4542 | 135.5331 | 45.7425 | BLLAC | 0.243 | 0.048 | 5 | 7,8,11,12b,13 |
| J0901.5+6711 | 135.3910 | 67.2214 | UNCL | 0.566 | 0.075 | 3 | 3,4,13 |
| J0902.4+2051 | 135.6121 | 20.8462 | BLLAC | 0.560 | 0.459 | 2 | 3,13 |
| J0902.4+6440 | 135.7258 | 64.7441 | BLLAC | 1.158 | 0.714 | 3 | 1,3,13 |
| J0903.1+4652 | 135.7666 | 46.8511 | FSRQ | 0.743 | 0.463 | 4 | 1,3,6,13 |
| J0904.0+2724 | 135.8876 | 27.3244 | FSRQ | 1.026 | 0.688 | 4 | 1,3,6,13 |
| J0904.6+4238 | 136.0651 | 42.6347 | FSRQ | 0.877 | 0.377 | 3 | 1,3,13 |
| J0905.6+1358 | 136.3958 | 13.9684 | BLLAC | 1.063 | 1.267 | 2 | 3,13 |
| J0906.2−1707 | 136.5905 | −17.1068 | UNCL | 0.413 | 0.091 | 3 | 3,4,6 |
| J0906.3−0905 | 136.5752 | −9.0958 | BLLAC | 0.864 | 0.585 | 2 | 3,13 |
| J0906.7+4950 | 136.7146 | 49.8767 | FSRQ | 0.701 | 0.441 | 4 | 3,7,8,13 |
| J0908.9+2311 | 137.2526 | 23.1869 | BLLAC | 0.539 | 0.542 | 3 | 3,6,13 |
| J0909.1+0121 | 137.2920 | 1.3599 | FSRQ | 0.569 | 0.712 | 2 | 3,13 |
| J0909.6+0159 | 137.4160 | 2.0015 | BLLAC | 0.546 | 0.370 | 3 | 1,3,13 |
| J0909.7+3104 | 137.4720 | 31.1009 | BLLAC | 0.139 | 0.036 | 7 | 5,6,7,8,11,12b,13 |
| J0909.7−0230 | 137.4372 | −2.5251 | FSRQ | 0.571 | 0.193 | 3 | 1,6,13 |
| J0910.0+4257 | 137.3896 | 42.8962 | CLAGN | 0.374 | 0.202 | 5 | 1,3,6,12b,13 |
| J0910.6+2247 | 137.6756 | 22.8099 | FSRQ | 0.910 | 0.137 | 3 | 1,3,13 |
| J0910.6+3329 | 137.6543 | 33.4901 | BLLAC | 0.609 | 0.774 | 2 | 3,13 |
| J0910.8+3859 | 137.7168 | 39.0339 | BLLAC | 0.217 | 0.166 | 3 | 3,6,13 |
| J0911.7+3349 | 137.9490 | 33.8213 | BLLAC | 0.298 | 0.106 | 5 | 3,7,8,12b,13 |
| J0912.2+2800 | 138.0467 | 27.9911 | BLLAC | 0.903 | 0.715 | 3 | 1,3,13 |
| J0912.2+4127 | 138.0484 | 41.4359 | FSRQ | 0.816 | 0.239 | 3 | 1,3,13 |
| J0912.2−2751 | 138.1316 | −27.8714 | UNCL | 1.754 | 0.061 | 2 | 3,4 |
| J0912.5+1556 | 138.1275 | 15.9244 | BLLAC | 0.155 | 0.025 | 3 | 11,12b,13 |
| J0912.9−2102 | 138.2509 | −21.0558 | BLLAC | 0.074 | 0.018 | 2 | 5,6 |
| J0913.3+8133 | 138.3424 | 81.5516 | BLLAC | 0.540 | 0.224 | 4 | 1,6,12b,13 |
| J0914.1−0202 | 138.5344 | −1.9959 | UNCL | 0.519 | 0.183 | 3 | 1,4,13 |
| J0914.4+0249 | 138.6580 | 2.7665 | FSRQ | 0.543 | 0.183 | 4 | 1,3,12c,13 |
| J0915.4−3027 | 138.9204 | −30.4971 | UNCL | - | - | - | |
| J0915.9+2933 | 138.9683 | 29.5567 | BLLAC | 0.035 | - | 1 | 13 |
| J0916.7+3856 | 139.2038 | 38.9078 | FSRQ | 1.064 | 0.859 | 3 | 1,3,13 |
| J0916.7+5238 | 139.2164 | 52.6412 | BLLAC | 0.133 | 0.035 | 7 | 5,6,7,8,11,12b,13 |
| J0917.1−2131 | 139.3626 | −21.5262 | FSRQ | 0.950 | - | 1 | 3 |
| J0917.3−0342 | 139.3108 | −3.7207 | BLLAC | 0.172 | 0.023 | 3 | 6,12b,13 |
| J0918.9−0625 | 139.6665 | −6.4747 | UNCL | 0.783 | 0.133 | 4 | 3,4,12b,13 |
| J0919.3−2202 | 139.8593 | −22.0119 | UNCL | 0.491 | 0.159 | 3 | 3,4,6 |
| J0920.3−0443 | 140.1234 | −4.6599 | UNCL | 0.896 | 0.417 | 3 | 3,4,13 |
| J0920.9+4441 | 140.2436 | 44.6983 | FSRQ | 0.560 | 0.598 | 3 | 3,6,13 |
| J0920.9−2256 | 140.2395 | −22.9560 | UNCL | 0.181 | - | 1 | 6 |
| J0921.6+6216 | 140.4010 | 62.2645 | FSRQ | 0.942 | 0.614 | 3 | 1,3,13 |
| J0921.7+2336 | 140.4391 | 23.5967 | BLLAC | 0.555 | 0.372 | 3 | 1,3,13 |
| J0922.4−0528 | 140.5986 | −5.4853 | AMB | 0.480 | 0.341 | 3 | 3,6,13 |
| J0922.6+0434 | 140.6136 | 4.5608 | UNCL | 0.656 | 0.317 | 4 | 1,3,11,13 |
| J0922.6+4454 | 140.6459 | 44.9636 | SEY | 0.904 | 0.656 | 5 | 1,3,6,12b,13 |
| J0923.5+3852 | 140.8102 | 38.8278 | UNCL | 0.790 | 0.204 | 2 | 11,13 |
| J0923.5+4125 | 140.8804 | 41.4243 | FSRQ | 0.639 | 0.176 | 3 | 1,3,13 |
| J0924.0+0534 | 141.0043 | 5.5626 | BLLAC | 0.432 | 0.273 | 4 | 1,3,6,13 |
| J0924.0+2816 | 140.9647 | 28.2570 | FSRQ | 0.651 | 0.253 | 4 | 1,3,6,13 |
| J0925.7+3126 | 141.4319 | 31.4530 | BLLAC | 0.391 | 0.120 | 4 | 1,3,6,13 |
| J0925.7+5959 | 141.4287 | 59.9713 | BLLAC | 1.185 | 0.811 | 3 | 3,4,13 |
| J0926.4+5412 | 141.6620 | 54.1907 | BLLAC | 0.608 | 0.225 | 3 | 1,3,13 |
| J0927.2+2454 | 141.8453 | 24.9370 | BLLAC | 0.649 | 0.338 | 3 | 1,3,13 |
| J0928.1−2035 | 141.9659 | −20.5809 | FSRQ | 0.341 | 0.215 | 2 | 3,6 |
| J0928.2−3048 | 142.1416 | −30.8289 | UNCL | - | - | - | |
| J0928.4−0415 | 142.1395 | −4.1525 | UNCL | 0.733 | 0.089 | 3 | 3,4,13 |
| J0928.5+4048 | 142.1560 | 40.8126 | BLLAC | 0.747 | 0.419 | 3 | 1,3,13 |
| J0928.7−3529 | 142.2076 | −35.4969 | UNCL | - | - | - | |
| J0929.3+5014 | 142.3143 | 50.2267 | BLLAC | 0.339 | 0.327 | 2 | 3,13 |
| J0929.3−2414 | 142.3677 | −24.2758 | BLLAC | 0.152 | 0.039 | 3 | 3,6,11 |
| J0929.6+4621 | 142.3448 | 46.3462 | UNCL | 0.439 | 0.161 | 6 | 3,4,6,7,8,13 |
| J0930.3+8612 | 142.4294 | 86.2059 | BLLAC | 1.347 | - | 1 | 3 |
| J0930.5+4951 | 142.6566 | 49.8404 | BLLAC | 0.158 | 0.048 | 5 | 6,7,8,12b,13 |
| J0930.7+3502 | 142.7303 | 35.0604 | BLLAC | 0.978 | 0.074 | 2 | 3,13 |
| J0930.9+0033 | 142.7177 | 0.5830 | FSRQ | 0.742 | 0.228 | 3 | 1,3,13 |
| J0930.9−1015 | 142.7613 | −10.2236 | UNCL | 0.536 | 0.084 | 3 | 3,4,6 |
| J0931.2−8533 | 142.6357 | −85.5666 | UNCL | 0.205 | - | 1 | 6 |
| J0931.9+6737 | 142.9870 | 67.6147 | BLLAC | 0.879 | 0.755 | 4 | 1,3,6,13 |
| J0932.6+5306 | 143.1715 | 53.1094 | NLS1 | 0.560 | 0.378 | 3 | 1,3,13 |
| J0932.7+1041 | 143.1640 | 10.7098 | BLLAC | 0.192 | 0.041 | 5 | 6,7,8,12b,13 |
| J0934.3+3926 | 143.5278 | 39.4423 | BLLAC | 0.748 | 0.258 | 3 | 1,3,13 |
| J0934.5−1720 | 143.6257 | −17.3560 | BLLAC | 0.177 | 0.025 | 3 | 11,12b,13 |
| J0935.3−1736 | 143.8116 | −17.6163 | BLLAC | 0.341 | 0.211 | 4 | 3,4,6,13 |
| J0936.3−2111 | 144.0562 | −21.1952 | UNCL | 0.699 | - | 1 | 11 |
| J0936.5+1847 | 144.1153 | 18.8343 | BLLAC | 0.561 | 0.274 | 4 | 1,3,6,13 |
| J0937.1+5008 | 144.3014 | 50.1478 | SEY | 0.384 | 0.216 | 4 | 1,3,6,13 |
| J0937.9−1434 | 144.4780 | −14.5640 | BLLAC | 0.305 | - | 1 | 6 |
| J0939.3−1732 | 144.8300 | −17.5266 | FSRQ | 0.784 | 0.496 | 2 | 3,13 |
| J0940.0−2828 | 145.0204 | −28.4916 | UNCL | - | - | - | |
| J0940.4+6148 | 145.0936 | 61.8073 | BLLAC | 0.168 | 0.033 | 5 | 6,7,8,12b,13 |
| J0940.9−1335 | 145.2606 | −13.5975 | FSRQ | 0.515 | 0.439 | 2 | 3,6 |
| J0941.7+4125 | 145.4569 | 41.3513 | FSRQ | 0.606 | 0.096 | 3 | 1,3,13 |
| J0941.9+2724 | 145.4684 | 27.3716 | BLLAC | 0.546 | 0.217 | 4 | 1,3,6,13 |
| J0942.3+2842 | 145.5971 | 28.7373 | BLLAC | 0.329 | 0.077 | 7 | 3,6,7,8,11,12b,13 |
| J0942.3−0800 | 145.5894 | −7.9981 | BLLAC | 0.531 | 0.390 | 3 | 3,6,13 |
| J0943.7+6137 | 146.0852 | 61.5973 | FSRQ | 0.686 | 0.442 | 3 | 1,3,13 |
| J0944.2+5557 | 146.1728 | 55.9647 | BLLAC | 0.423 | 0.216 | 3 | 1,3,13 |
| J0945.2+5200 | 146.2173 | 52.0428 | FSRQ | 0.676 | 0.439 | 3 | 1,3,13 |
| J0945.5+4635 | 146.4254 | 46.6141 | MIS | 0.645 | 0.059 | 6 | 3,7,8,11,12b,13 |
| J0945.7+5759 | 146.4260 | 57.9632 | BLLAC | 0.216 | 0.239 | 7 | 3,5,6,7,8,10,13 |
| J0946.0+4735 | 146.5186 | 47.5862 | BLLAC | 0.575 | 0.140 | 3 | 1,3,13 |
| J0946.2+0104 | 146.5842 | 1.0811 | BLLAC | 0.457 | 0.213 | 5 | 1,8,12b,12c,13 |
| J0946.6+1016 | 146.6461 | 10.2850 | FSRQ | 0.895 | 0.179 | 3 | 1,3,13 |
| J0947.1−2541 | 146.7897 | −25.6833 | UNCL | - | - | - | |
| J0947.6+2215 | 146.9108 | 22.2593 | BLLAC | 0.498 | 0.072 | 3 | 1,3,13 |
| J0947.9+1121 | 146.9412 | 11.3392 | BLLAC | 0.176 | 0.034 | 5 | 7,8,11,12b,13 |
| J0948.6−0338 | 147.1836 | −3.6404 | UNCL | 0.882 | 0.249 | 4 | 3,4,6,13 |
| J0948.9+0022 | 147.2388 | 0.3738 | NLS1 | 0.409 | 0.273 | 4 | 1,3,6,13 |
| J0949.0+4038 | 147.2306 | 40.6624 | FSRQ | 0.621 | 0.750 | 2 | 3,13 |
| J0949.2+1749 | 147.4157 | 17.8804 | FSRQ | 0.702 | 0.119 | 3 | 3,6,13 |
| J0949.7+5819 | 147.4159 | 58.3203 | FSRQ | 0.820 | 0.499 | 2 | 1,13 |
| J0950.2+0615 | 147.5144 | 6.2511 | BLLAC | 0.615 | 0.383 | 4 | 1,3,8,13 |
| J0950.2+4553 | 147.5492 | 45.8889 | BLLAC | 0.409 | 0.245 | 3 | 1,3,13 |
| J0952.1+3932 | 148.0613 | 39.6044 | BLLAC | 0.777 | 0.374 | 3 | 1,3,13 |
| J0952.2+7503 | 148.1006 | 75.0371 | BLLAC | 0.175 | 0.035 | 4 | 6,11,12b,13 |
| J0952.8+0712 | 148.2066 | 7.2250 | BLLAC | 0.507 | 0.135 | 4 | 1,3,6,13 |
| J0953.0−0840 | 148.2613 | −8.6718 | BLLAC | 0.743 | 0.891 | 2 | 3,13 |
| J0953.4−7659 | 148.2681 | −76.9672 | BLLAC | 0.130 | - | 1 | 6 |
| J0954.2+4913 | 148.5408 | 49.2497 | BLLAC | 0.964 | 0.706 | 3 | 1,3,13 |
| J0955.1+3551 | 148.7828 | 35.8502 | BLLAC | 0.405 | 0.169 | 5 | 6,7,8,12b,13 |
| J0955.2+0835 | 148.7578 | 8.5617 | BLLAC | 0.630 | 0.267 | 4 | 1,3,6,13 |
| J0956.0+3936 | 149.0357 | 39.5878 | FSRQ | 1.233 | 0.072 | 3 | 1,3,13 |
| J0956.5−0958 | 149.1176 | −9.9553 | BLLAC | 0.140 | 0.032 | 3 | 5,6,11 |
| J0956.7+2516 | 149.2078 | 25.2545 | FSRQ | 0.517 | 0.329 | 3 | 1,3,13 |
| J0957.3−1348 | 149.3258 | −13.8337 | FSRQ | 0.617 | 0.548 | 2 | 3,6 |
| J0957.6+5523 | 149.4091 | 55.3827 | FSRQ | 0.552 | 0.610 | 2 | 3,13 |
| J0957.8+3423 | 149.4437 | 34.3709 | BLLAC | 0.279 | 0.214 | 2 | 6,13 |
| J0958.0+3222 | 149.5873 | 32.4006 | NLS1 | 1.344 | 1.776 | 2 | 3,13 |
| J0958.0+4728 | 149.5820 | 47.4188 | FSRQ | 1.144 | 0.738 | 3 | 1,3,13 |
| J0958.0−0319 | 149.5250 | −3.2945 | BLLAC | 0.554 | 0.117 | 4 | 1,3,4,13 |
| J0958.1−6753 | 149.5544 | −67.8785 | UNCL | 0.174 | 0.035 | 2 | 4,6 |
| J0958.3−2656 | 149.6025 | −26.9267 | AMB | 0.006 | 0.004 | 2 | 5,6 |
| J0958.4+5042 | 149.6575 | 50.6660 | FSRQ | 0.832 | 0.519 | 3 | 1,3,13 |
| J0958.4−2441 | 149.5853 | −24.7332 | UNCL | 0.986 | 0.019 | 2 | 3,4 |
| J0958.7+6534 | 149.6969 | 65.5652 | BLLAC | 0.588 | 0.648 | 2 | 3,13 |
| J0958.8+7039 | 149.7076 | 70.6665 | UNCL | 0.240 | 0.050 | 5 | 4,6,11,12b,13 |
| J0959.4+2120 | 149.8745 | 21.3892 | BLLAC | 0.228 | 0.070 | 6 | 3,6,7,8,12b,13 |
| J0959.6+4606 | 149.8325 | 46.0644 | SEY | 0.167 | 0.010 | 5 | 3,6,11,12b,13 |
| J1001.1+2911 | 150.2925 | 29.1938 | FSRQ | 1.010 | 0.548 | 2 | 3,13 |
| J1002.5+2215 | 150.6434 | 22.2708 | BLLAC | 0.616 | 0.328 | 4 | 1,3,6,13 |
| J1003.4+0205 | 150.8608 | 2.0822 | BLLAC | 0.786 | 0.617 | 3 | 1,3,13 |
| J1003.6+2605 | 150.9260 | 26.0869 | BLLAC | 0.606 | 0.141 | 3 | 1,3,13 |
| J1003.6−2137 | 150.9287 | −21.6359 | UNCL | 0.149 | 0.024 | 6 | 4,5,6,11,12b,13 |
| J1006.5+6440 | 151.5509 | 64.6699 | BLLAC | 0.732 | 0.727 | 3 | 1,3,13 |
| J1006.7−2159 | 151.6934 | −21.9890 | FSRQ | 0.159 | 0.046 | 3 | 3,6,13 |
| J1007.0+3455 | 151.7353 | 34.9126 | BLLAC | 0.640 | 0.537 | 3 | 1,3,13 |
| J1007.6−3332 | 151.8808 | −33.5519 | FSRQ | 0.575 | - | 1 | 6 |
| J1008.0+0028 | 152.0477 | 0.5000 | MIS | 0.076 | 0.022 | 10 | 3,5,6,7,8,10,11,12b,12c,13 |
| J1008.0+0620 | 152.0034 | 6.3559 | BLLAC | 0.389 | 0.363 | 3 | 3,6,13 |
| J1008.1+4706 | 152.0475 | 47.0892 | BLLAC | 0.294 | 0.045 | 5 | 6,7,8,12b,13 |
| J1008.7−2909 | 152.1880 | −29.2122 | UNCL | 1.670 | - | 1 | 3 |
| J1008.8−3139 | 152.2106 | −31.6515 | BLLAC | 0.542 | 0.211 | 2 | 4,6 |
| J1010.2−3119 | 152.5666 | −31.3190 | BLLAC | 0.100 | 0.023 | 2 | 5,6 |
| J1010.8−0158 | 152.7153 | −2.0054 | FSRQ | 0.590 | 0.408 | 3 | 1,3,13 |
| J1011.3−0427 | 152.8760 | −4.3910 | FSRQ | 0.970 | 1.185 | 2 | 3,13 |
| J1012.3+0629 | 153.0556 | 6.5159 | AMB | 0.664 | 0.711 | 2 | 3,13 |
| J1012.3−1232 | 153.0627 | −12.5611 | UNCL | 0.853 | 0.203 | 2 | 3,4 |
| J1012.7+2439 | 153.1724 | 24.6565 | FSRQ | 1.433 | 0.552 | 3 | 1,3,13 |
| J1012.7+4228 | 153.1846 | 42.4992 | MIS | 0.229 | 0.132 | 4 | 1,6,12b,13 |
| J1013.3−2551 | 153.3046 | −25.7819 | UNCL | 1.584 | - | 1 | 3 |
| J1013.4−4006 | 153.3315 | −40.0966 | UNCL | - | - | - | |
| J1013.7+3444 | 153.4567 | 34.7641 | FSRQ | 0.765 | 0.478 | 3 | 1,3,13 |
| J1014.3+4112 | 153.5745 | 41.2049 | UNCL | 0.732 | 0.214 | 5 | 3,4,7,8,13 |
| J1014.8+2257 | 153.6961 | 23.0213 | FSRQ | 0.684 | 0.874 | 2 | 3,13 |
| J1014.8−0537 | 153.6919 | −5.6797 | UNCL | 0.589 | 0.364 | 3 | 3,4,13 |
| J1015.0+4926 | 153.7672 | 49.4335 | BLLAC | 0.270 | 0.281 | 4 | 3,4,6,13 |
| J1015.6+5553 | 153.9351 | 55.8502 | FSRQ | 0.963 | 0.177 | 3 | 1,3,13 |
| J1016.0+0512 | 154.0131 | 5.2173 | FSRQ | 1.311 | 0.414 | 3 | 1,3,13 |
| J1016.4+7703 | 154.2024 | 77.0455 | UNCL | 0.683 | 0.161 | 3 | 3,4,13 |
| J1016.5−2650 | 154.1446 | −26.8499 | UNCL | 0.690 | 0.014 | 2 | 3,4 |
| J1017.3+5204 | 154.2778 | 52.0464 | BLLAC | 0.282 | 0.090 | 6 | 3,6,7,8,12b,13 |
| J1017.4+2538 | 154.3516 | 25.6656 | BLLAC | 0.278 | 0.063 | 6 | 6,7,8,11,12b,13 |
| J1017.8+0715 | 154.5887 | 7.2521 | FSRQ | 0.739 | 0.223 | 4 | 1,3,6,13 |
| J1018.1+1905 | 154.5330 | 19.1043 | BLLAC | 0.584 | 0.230 | 3 | 1,3,13 |
| J1018.3−3124 | 154.6198 | −31.3983 | FSRQ | - | - | - | |
| J1018.4+0528 | 154.6160 | 5.5083 | FSRQ | 1.261 | 0.428 | 3 | 1,3,13 |
| J1018.4+3540 | 154.5458 | 35.7110 | FSRQ | 0.857 | 0.551 | 3 | 1,3,13 |
| J1018.8+5913 | 154.7439 | 59.1911 | BLLAC | 0.664 | 0.302 | 2 | 3,13 |
| J1018.9+1043 | 154.7416 | 10.6071 | AMB | 0.662 | 0.191 | 3 | 1,3,13 |
| J1019.7+6321 | 154.9620 | 63.3338 | BLLAC | 0.452 | 0.240 | 3 | 1,3,13 |
| J1021.1+1626 | 155.2515 | 16.4317 | BLLAC | 0.566 | 0.245 | 3 | 1,3,13 |
| J1021.4+8021 | 155.5088 | 80.3972 | UNCL | 0.771 | 0.429 | 4 | 3,7,8,13 |
| J1021.9+5123 | 155.5526 | 51.4001 | AMB | 0.153 | 0.021 | 6 | 6,7,8,11,12b,13 |
| J1022.4−4231 | 155.5766 | −42.5353 | UNCL | - | - | - | |
| J1022.7−0112 | 155.6822 | −1.2173 | BLLAC | 0.117 | - | 1 | 13 |
| J1023.1+3949 | 155.7982 | 39.8043 | FSRQ | 0.864 | 0.529 | 3 | 1,3,13 |
| J1023.2+2859 | 155.8502 | 28.9475 | FSRQ | 0.556 | 0.144 | 5 | 3,6,7,8,13 |
| J1023.8+3002 | 155.9156 | 30.0160 | BLLAC | 0.275 | 0.213 | 2 | 1,13 |
| J1023.8−4335 | 155.9850 | −43.6006 | BLLAC | - | - | - | |
| J1023.9−3236 | 156.0018 | −32.5711 | FSRQ | - | - | - | |
| J1024.8+2332 | 156.2235 | 23.5428 | SEY | 0.219 | 0.202 | 6 | 3,6,7,8,11,13 |
| J1026.9+0608 | 156.7642 | 6.1594 | BLLAC | 0.302 | 0.070 | 5 | 6,7,8,12b,13 |
| J1026.9−1749 | 156.7441 | −17.8164 | BLLAC | 0.118 | - | 1 | 6 |
| J1027.0−8542 | 156.6432 | −85.7206 | BLLAC | - | - | - | |
| J1027.2+7427 | 156.8506 | 74.4739 | FSRQ | 0.679 | 0.216 | 2 | 3,13 |
| J1027.6+1828 | 156.9376 | 18.5274 | UNCL | 0.461 | 0.207 | 4 | 1,3,4,13 |
| J1027.6+6317 | 156.8540 | 63.2981 | BLLAC | 0.816 | 0.652 | 3 | 1,3,13 |
| J1027.6+8251 | 157.1750 | 82.8946 | UNCL | 0.875 | 0.307 | 3 | 3,4,13 |
| J1027.9+0252 | 157.0850 | 2.9229 | FSRQ | 0.663 | 0.132 | 7 | 3,6,7,8,12b,12c,13 |
| J1028.3+3108 | 157.0734 | 31.1262 | BLLAC | 0.237 | 0.031 | 6 | 3,6,7,8,12b,13 |
| J1028.4−0234 | 157.1418 | −2.6166 | FSRQ | 0.934 | 0.318 | 4 | 1,3,12b,13 |
| J1030.2−8403 | 157.5637 | −84.0524 | UNCL | - | - | - | |
| J1030.4−3001 | 157.6292 | −30.0613 | UNCL | 0.584 | 0.047 | 3 | 6,12b,13 |
| J1030.6−2028 | 157.6684 | −20.5101 | BLLAC | 0.877 | 0.770 | 2 | 3,4 |
| J1031.1+7442 | 157.8418 | 74.6995 | FSRQ | 0.107 | - | 1 | 13 |
| J1031.3+5053 | 157.8272 | 50.8933 | BLLAC | 0.106 | 0.046 | 3 | 5,6,13 |
| J1031.6+6019 | 157.9365 | 60.3418 | FSRQ | 0.930 | 0.562 | 3 | 1,3,13 |
| J1031.8−2609 | 157.9079 | −26.1213 | UNCL | 0.219 | 0.043 | 5 | 4,6,11,12b,13 |
| J1032.6+3737 | 158.1697 | 37.6408 | BLLAC | 0.502 | 0.501 | 2 | 3,13 |
| J1032.7+6624 | 158.1628 | 66.3898 | BLLAC | 0.681 | 0.410 | 3 | 1,3,13 |
| J1033.1+4115 | 158.2654 | 41.2684 | FSRQ | 0.320 | 0.167 | 3 | 1,3,13 |
| J1033.5+4221 | 158.3246 | 42.3764 | BLLAC | 0.194 | 0.034 | 7 | 5,6,7,8,11,12b,13 |
| J1033.7+3708 | 158.4433 | 37.1403 | BLLAC | 0.333 | 0.075 | 6 | 6,7,8,11,12b,13 |
| J1033.9+6050 | 158.4643 | 60.8520 | FSRQ | 0.744 | 0.452 | 4 | 1,3,6,13 |
| J1034.0−2547 | 158.4627 | −25.7522 | UNCL | 1.135 | 0.321 | 2 | 3,13 |
| J1035.3+5541 | 158.9398 | 55.7151 | BLLAC | 0.883 | 0.268 | 3 | 1,3,13 |
| J1035.3−2050 | 158.8137 | −20.8406 | UNCL | - | - | - | |
| J1036.2+2202 | 159.1374 | 22.0534 | FSRQ | 0.633 | 0.457 | 3 | 1,3,13 |
| J1036.5+1231 | 159.1682 | 12.5607 | BLLAC | 0.529 | 0.369 | 3 | 1,3,13 |
| J1036.6−3741 | 159.2227 | −37.7375 | FSRQ | - | - | - | |
| J1037.0−1954 | 159.2332 | −19.9066 | UNCL | 0.302 | 0.003 | 2 | 4,6 |
| J1037.4−2933 | 159.3170 | −29.5674 | CLAGN | 0.351 | 0.326 | 2 | 3,13 |
| J1037.7+5711 | 159.4346 | 57.1988 | BLLAC | 1.137 | 1.393 | 2 | 3,13 |
| J1037.7−2822 | 159.4269 | −28.3845 | FSRQ | 1.028 | - | 1 | 3 |
| J1038.2−2425 | 159.6003 | −24.3986 | UNCL | 1.007 | 0.372 | 3 | 3,12b,13 |
| J1038.5+3926 | 159.6912 | 39.4597 | BLLAC | 0.490 | 0.297 | 3 | 1,3,13 |
| J1039.6+0535 | 159.9196 | 5.6025 | BLLAC | 0.361 | 0.109 | 5 | 6,7,8,12b,13 |
| J1039.7−1540 | 159.7779 | −15.6852 | FSRQ | 0.615 | 0.076 | 2 | 3,6 |
| J1039.9+7326 | 159.9146 | 73.4325 | UNCL | 0.666 | 0.447 | 3 | 3,4,13 |
| J1040.5+0617 | 160.1318 | 6.2894 | BLLAC | 1.114 | 0.735 | 4 | 1,3,8,13 |
| J1041.0+1342 | 160.2432 | 13.6974 | UNCL | 1.156 | 1.051 | 2 | 1,3 |
| J1041.1−1201 | 160.2857 | −12.0586 | UNCL | 0.347 | 0.071 | 3 | 3,4,6 |
| J1041.7+3902 | 160.4548 | 39.0221 | BLLAC | 0.169 | 0.035 | 8 | 5,6,7,8,10,11,12b,13 |
| J1041.9−0557 | 160.5179 | −5.9713 | BLLAC | 0.167 | 0.038 | 4 | 6,11,12b,13 |
| J1042.1−4128 | 160.5126 | −41.4916 | UNCL | 0.300 | - | 1 | 4 |
| J1042.9+0054 | 160.7660 | 0.9057 | BLLAC | 0.329 | 0.187 | 5 | 6,7,8,12c,13 |
| J1043.2+2408 | 160.7876 | 24.1432 | CLAGN | 0.411 | 0.416 | 2 | 3,13 |
| J1043.6+0654 | 160.8495 | 6.8861 | BLLAC | 1.213 | 0.859 | 3 | 1,3,13 |
| J1044.6+8053 | 161.0961 | 80.9110 | FSRQ | 0.683 | 0.379 | 2 | 3,13 |
| J1045.3+2751 | 161.3179 | 27.8593 | BLLAC | 0.842 | 0.519 | 4 | 1,3,4,13 |
| J1045.8−2928 | 161.4193 | −29.4573 | FSRQ | 0.680 | 0.199 | 2 | 3,6 |
| J1046.0+5448 | 161.6200 | 54.8290 | AMB | 0.196 | 0.032 | 5 | 7,8,11,12b,13 |
| J1046.8−2534 | 161.7142 | −25.5958 | BLLAC | 0.182 | 0.021 | 3 | 6,12b,13 |
| J1047.7+7238 | 161.9480 | 72.6369 | BLLAC | 0.437 | 0.374 | 3 | 3,6,13 |
| J1047.9+0055 | 162.0323 | 0.9287 | AMB | 0.632 | 0.163 | 6 | 1,3,6,12b,12c,13 |
| J1047.9−3738 | 161.9872 | −37.6252 | UNCL | - | - | - | |
| J1048.0−1912 | 162.0276 | −19.1599 | NLS1 | 0.847 | - | 1 | 3 |
| J1048.4+7143 | 162.1151 | 71.7266 | FSRQ | 0.692 | 0.782 | 2 | 3,13 |
| J1049.5+1548 | 162.4140 | 15.8104 | BLLAC | 0.136 | - | 1 | 13 |
| J1049.7+5011 | 162.2400 | 50.1625 | BLLAC | 0.305 | 0.096 | 6 | 3,6,7,8,12b,13 |
| J1049.8+1429 | 162.4430 | 14.4940 | UNCL | 0.949 | 0.371 | 3 | 1,3,13 |
| J1050.1+0432 | 162.5419 | 4.5470 | FSRQ | 0.822 | 0.552 | 3 | 1,3,13 |
| J1051.4+3942 | 162.8557 | 39.7238 | BLLAC | 0.344 | 0.188 | 4 | 1,3,6,13 |
| J1051.4−3139 | 162.7699 | −31.6373 | FSRQ | - | - | - | |
| J1051.6+2109 | 162.9533 | 21.3312 | FSRQ | 0.975 | 0.499 | 4 | 1,3,4,13 |
| J1051.9+0103 | 162.9660 | 1.0530 | BLLAC | 0.408 | 0.218 | 6 | 1,3,6,8,12b,13 |
| J1052.3+0818 | 163.1022 | 8.2360 | BLLAC | 0.200 | 0.042 | 6 | 6,7,8,11,12b,13 |
| J1052.9−3743 | 163.2421 | −37.7218 | BLLAC | - | - | - | |
| J1053.7+4930 | 163.4339 | 49.4989 | MIS | 0.095 | 0.020 | 8 | 5,6,7,8,10,11,12b,13 |
| J1053.9+8628 | 163.5928 | 86.4934 | UNCL | 0.224 | 0.129 | 4 | 3,5,6,11 |
| J1054.2+3926 | 163.6351 | 39.4701 | FSRQ | 0.865 | 0.353 | 3 | 1,3,13 |
| J1054.5+2211 | 163.6276 | 22.1819 | BLLAC | 0.317 | 0.270 | 2 | 3,13 |
| J1055.5−0125 | 163.8932 | −1.4379 | BLLAC | 0.755 | 0.591 | 4 | 1,3,4,13 |
| J1056.0+0253 | 164.0275 | 2.8704 | BLLAC | 0.188 | 0.054 | 7 | 6,7,8,11,12b,12c,13 |
| J1056.8+7012 | 164.2234 | 70.1961 | FSRQ | 0.657 | 0.494 | 3 | 3,6,13 |
| J1057.2+5510 | 164.2810 | 55.1756 | BLLAC | 0.761 | 0.740 | 3 | 1,3,13 |
| J1057.3−2341 | 164.3518 | −23.7005 | FSRQ | 1.718 | - | 1 | 3 |
| J1057.8−2754 | 164.4615 | −27.9030 | BLLAC | 0.088 | 0.047 | 5 | 5,6,11,12b,13 |
| J1058.0+4305 | 164.5122 | 43.0782 | BLLAC | 1.102 | 0.649 | 4 | 1,3,6,13 |
| J1058.4+0133 | 164.6234 | 1.5663 | FSRQ | 0.615 | 0.620 | 2 | 3,13 |
| J1058.5+8115 | 164.5481 | 81.2424 | FSRQ | 0.530 | 0.155 | 3 | 3,6,13 |
| J1058.6+2817 | 164.6246 | 28.2962 | BLLAC | 0.255 | 0.234 | 2 | 1,13 |
| J1058.6+5627 | 164.6572 | 56.4698 | BLLAC | 0.308 | 0.381 | 4 | 3,6,7,13 |
| J1058.6−8003 | 164.6805 | −80.0650 | BLLAC | - | - | - | |
| J1059.2−1134 | 164.8018 | −11.5730 | BLLAC | 0.611 | - | 1 | 3 |
| J1059.5+2057 | 164.9127 | 20.9561 | FSRQ | 0.716 | 0.397 | 4 | 1,3,6,13 |
| J1100.3+4020 | 165.0878 | 40.3245 | BLLAC | 0.326 | 0.278 | 2 | 3,13 |
| J1101.4+4108 | 165.3530 | 41.1465 | BLLAC | 1.152 | 1.293 | 3 | 1,3,13 |
| J1101.5+3904 | 165.3753 | 39.0757 | UNCL | 0.941 | - | 1 | 13 |
| J1102.1+2249 | 165.5131 | 22.6989 | UNCL | 0.577 | 0.206 | 3 | 6,11,13 |
| J1102.6+5251 | 165.7077 | 52.8368 | NLS1 | 0.665 | 0.173 | 3 | 1,3,13 |
| J1102.8−0148 | 165.7209 | −1.8185 | UNCL | 0.545 | 0.152 | 5 | 1,3,4,6,12c |
| J1102.9+3014 | 165.8054 | 30.2452 | FSRQ | 0.236 | 0.129 | 5 | 3,6,7,8,13 |
| J1103.0+1157 | 165.7647 | 11.9713 | FSRQ | 0.655 | 0.403 | 3 | 1,3,13 |
| J1103.6−2329 | 165.9067 | −23.4920 | BLLAC | 0.093 | 0.009 | 2 | 5,6 |
| J1104.0+0020 | 165.9840 | 0.3768 | BLLAC | 0.192 | 0.042 | 7 | 6,7,8,11,12b,12c,13 |
| J1104.0+2611 | 165.9887 | 26.1886 | BLLAC | 0.771 | 0.312 | 3 | 1,3,13 |
| J1104.4+0730 | 166.1003 | 7.5148 | BLLAC | 0.296 | 0.240 | 2 | 3,13 |
| J1104.4+3812 | 166.1138 | 38.2088 | BLLAC | 0.082 | 0.082 | 2 | 11,13 |
| J1104.9+5748 | 166.0540 | 57.8702 | UNCL | - | - | - | |
| J1105.8+3944 | 166.4742 | 39.7825 | BLLAC | 0.122 | 0.009 | 6 | 5,6,10,11,12b,13 |
| J1106.0+2813 | 166.5303 | 28.2131 | FSRQ | 0.557 | 0.325 | 3 | 1,3,13 |
| J1106.2−1048 | 166.5234 | −10.8148 | UNCL | 0.242 | 0.062 | 2 | 6,11 |
| J1106.5−3646 | 166.6002 | −36.7830 | BLLAC | 0.412 | - | 1 | 6 |
| J1107.0−4449 | 166.7862 | −44.8188 | FSRQ | - | - | - | |
| J1107.6+0222 | 166.8996 | 2.3735 | BLLAC | 0.610 | 0.656 | 4 | 1,3,8,13 |
| J1107.7−3042 | 166.9339 | −30.7264 | FSRQ | - | - | - | |
| J1107.8+1501 | 166.9503 | 15.0363 | BLLAC | 0.386 | 0.178 | 4 | 1,4,6,13 |
| J1108.7−1844 | 167.1905 | −18.7515 | UNCL | 0.694 | 0.792 | 2 | 3,4 |
| J1109.3+2411 | 167.3174 | 24.1889 | BLLAC | 0.460 | 0.283 | 3 | 1,3,13 |
| J1109.6+3735 | 167.4104 | 37.6032 | BLLAC | 0.316 | 0.113 | 3 | 1,3,13 |
| J1109.7−4814 | 167.3286 | −48.2554 | UNCL | 0.513 | - | 1 | 6 |
| J1110.2+7135 | 167.6567 | 71.5657 | BLLAC | 0.579 | 0.643 | 2 | 3,13 |
| J1110.5−1836 | 167.6157 | −18.5980 | BLLAC | 0.860 | - | 1 | 3 |
| J1111.0+3542 | 167.7368 | 35.6520 | BLLAC | 0.549 | 0.401 | 3 | 1,3,13 |
| J1111.4−4624 | 167.8642 | −46.4178 | UNCL | - | - | - | |
| J1111.5+3455 | 167.8787 | 34.8676 | BLLAC | 0.864 | 0.577 | 3 | 1,3,13 |
| J1111.8+4858 | 167.9954 | 48.9504 | BLLAC | 0.577 | 0.149 | 5 | 1,3,4,12b,13 |
| J1112.4+1751 | 168.1025 | 17.8561 | BLLAC | 0.260 | 0.110 | 4 | 1,6,12b,13 |
| J1112.5+3448 | 168.1615 | 34.7775 | FSRQ | 1.125 | 0.133 | 3 | 1,3,13 |
| J1113.6−1920 | 168.4537 | −19.3815 | UNCL | 0.779 | 0.423 | 2 | 3,6 |
| J1114.5−0819 | 168.6356 | −8.2775 | FSRQ | 0.814 | - | 1 | 13 |
| J1114.7−0248 | 168.6653 | −2.7922 | FSRQ | 1.688 | 1.119 | 3 | 1,3,13 |
| J1115.2−0703 | 168.7989 | −7.0444 | UNCL | 0.437 | 0.169 | 4 | 3,4,6,13 |
| J1116.6+2915 | 169.1442 | 29.2548 | MIS | 0.048 | 0.012 | 6 | 5,6,10,11,12b,13 |
| J1117.0+2013 | 169.2760 | 20.2354 | BLLAC | 0.088 | 0.026 | 5 | 6,7,8,12b,13 |
| J1117.2+0008 | 169.3231 | 0.1093 | BLLAC | 0.267 | 0.107 | 6 | 6,7,8,12b,12c,13 |
| J1117.6+0217 | 169.3484 | 2.2721 | UNCL | 0.837 | 0.249 | 6 | 3,4,7,8,12b,13 |
| J1117.6+2550 | 169.4183 | 25.8130 | BLLAC | 0.282 | 0.121 | 4 | 3,6,12b,13 |
| J1117.7−3650 | 169.4934 | −36.8220 | UNCL | 0.677 | 0.164 | 2 | 4,6 |
| J1118.0+5356 | 169.4885 | 53.9319 | BLLAC | 0.936 | 1.090 | 2 | 3,13 |
| J1118.2−0415 | 169.5519 | −4.2234 | UNCL | 0.715 | 0.158 | 3 | 3,4,13 |
| J1118.2−4634 | 169.6123 | −46.5708 | FSRQ | - | - | - | |
| J1118.6−1235 | 169.5714 | −12.5484 | FSRQ | 1.718 | - | 1 | 3 |
| J1119.0+1235 | 169.7388 | 12.5783 | FSRQ | 1.566 | 0.706 | 3 | 1,3,13 |
| J1119.6−3047 | 169.9146 | −30.7889 | BLLAC | 0.233 | 0.081 | 2 | 6,11 |
| J1120.6+0713 | 170.1770 | 7.2198 | UNCL | - | - | - | - |
| J1120.8+4212 | 170.2003 | 42.2035 | BLLAC | 0.053 | - | 1 | 13 |
| J1121.3−0011 | 170.3309 | −0.2212 | MIS | 0.078 | 0.019 | 8 | 5,6,7,8,10,11,12b,13 |
| J1121.4−0553 | 170.3546 | −5.8990 | FSRQ | 0.623 | 0.443 | 3 | 3,6,13 |
| J1123.1−3233 | 170.8252 | −32.5385 | BLLAC | 0.200 | - | 1 | 6 |
| J1123.4−2529 | 170.8557 | −25.4825 | FSRQ | 0.143 | 0.021 | 3 | 3,5,6 |
| J1123.6+8028 | 170.9307 | 80.5065 | UNCL | 1.329 | 0.687 | 3 | 3,4,13 |
| J1123.8+7230 | 170.9550 | 72.5000 | BLLAC | 0.690 | 0.353 | 3 | 3,4,13 |
| J1124.0+2045 | 171.0223 | 20.7649 | BLLAC | 0.523 | 0.402 | 3 | 1,3,13 |
| J1124.0+2336 | 171.0113 | 23.6127 | CLAGN | 0.863 | 0.162 | 3 | 1,3,13 |
| J1124.4+2308 | 171.1316 | 23.1322 | BLLAC | 0.629 | 0.166 | 3 | 1,3,13 |
| J1124.6−0809 | 171.1563 | −8.1119 | UNCL | 0.638 | 0.447 | 3 | 3,4,13 |
| J1124.9+2143 | 171.2652 | 21.7167 | BLLAC | 1.002 | 0.722 | 4 | 1,3,4,13 |
| J1124.9+4934 | 171.2243 | 49.5694 | BLLAC | 0.520 | 0.411 | 4 | 1,3,4,13 |
| J1125.1−2101 | 171.2859 | −21.0183 | UNCL | 0.461 | 0.361 | 3 | 3,4,6 |
| J1125.5−3557 | 171.3812 | −35.9509 | BLLAC | 0.127 | - | 1 | 6 |
| J1125.9+2005 | 171.4948 | 20.0984 | AMB | 0.090 | 0.019 | 7 | 3,5,6,7,8,11,13 |
| J1125.9−0742 | 171.4666 | −7.7059 | BLLAC | 0.168 | 0.042 | 6 | 5,6,7,8,12b,13 |
| J1126.8−3829 | 171.6839 | −38.4789 | UNCL | 0.572 | - | 1 | 6 |
| J1127.0−1857 | 171.7683 | −18.9548 | FSRQ | 1.338 | - | 1 | 3 |
| J1127.4+5648 | 171.9172 | 56.8374 | FSRQ | 1.968 | 0.966 | 3 | 1,3,13 |
| J1127.6−4920 | 171.9191 | −49.3234 | UNCL | - | - | - | |
| J1127.8+3618 | 171.9953 | 36.3412 | FSRQ | 0.783 | 0.250 | 4 | 1,3,6,13 |
| J1128.0+5924 | 172.0556 | 59.4208 | FSRQ | 1.337 | 0.423 | 3 | 1,3,13 |
| J1128.8+3757 | 172.2635 | 37.9491 | BLLAC | 0.963 | 0.570 | 4 | 1,3,4,13 |
| J1129.1+3703 | 172.3096 | 37.0550 | BLLAC | 0.633 | 0.542 | 3 | 1,3,13 |
| J1129.2−0529 | 172.3086 | −5.4823 | FSRQ | 1.313 | 0.782 | 4 | 1,3,4,13 |
| J1129.2−1014 | 172.3022 | −10.2304 | UNCL | 0.817 | 0.407 | 2 | 3,6 |
| J1129.5+3034 | 172.4054 | 30.6096 | BLLAC | 0.586 | 0.213 | 3 | 1,3,13 |
| J1129.8−1447 | 172.5294 | −14.8243 | FSRQ | 1.200 | - | 1 | 3 |
| J1129.8−4217 | 172.5293 | −42.2447 | BLLAC | 0.150 | 0.003 | 2 | 5,6 |
| J1130.5−3137 | 172.6922 | −31.6354 | BLLAC | 0.159 | 0.004 | 2 | 5,6 |
| J1130.5−7801 | 172.6336 | −78.0182 | BLLAC | 0.167 | 0.044 | 2 | 4,6 |
| J1131.0+3815 | 172.7220 | 38.2552 | FSRQ | 1.082 | 0.631 | 3 | 1,3,13 |
| J1131.1−0944 | 172.7719 | −9.7351 | UNCL | 0.623 | 0.431 | 2 | 3,4 |
| J1131.4+5809 | 172.8276 | 58.1497 | BLLAC | 0.201 | 0.055 | 3 | 3,6,13 |
| J1131.4−0504 | 172.8772 | −5.0055 | MIS | 0.764 | 0.607 | 5 | 1,3,6,12b,13 |
| J1132.2−4736 | 173.0386 | −47.6482 | BLLAC | 0.196 | 0.005 | 3 | 4,5,6 |
| J1132.7+0034 | 173.1901 | 0.5744 | BLLAC | 0.529 | 0.488 | 2 | 3,13 |
| J1133.8−2048 | 173.4579 | −20.8144 | BLLAC | 0.068 | 0.014 | 3 | 5,6,11 |
| J1134.8−1729 | 173.6854 | −17.4839 | BLLAC | - | - | - | |
| J1135.1+3014 | 173.8087 | 30.1682 | BLLAC | 0.757 | 0.274 | 3 | 1,3,13 |
| J1135.7−0427 | 173.9926 | −4.4744 | FSRQ | 0.205 | 0.086 | 7 | 3,6,7,8,11,12b,13 |
| J1136.2+3407 | 174.1139 | 34.1276 | FSRQ | 1.336 | 0.284 | 3 | 1,3,13 |
| J1136.3−0501 | 174.0310 | −5.0325 | UNCL | 0.286 | 0.044 | 6 | 3,7,8,11,12b,13 |
| J1136.4+6736 | 174.1254 | 67.6179 | BLLAC | 0.098 | 0.024 | 7 | 5,6,7,8,11,12b,13 |
| J1136.4+7009 | 174.1100 | 70.1576 | BLLAC | 0.029 | 0.008 | 4 | 5,6,11,13 |
| J1136.8+2550 | 174.2089 | 25.8479 | SEY | 0.114 | 0.023 | 7 | 5,6,7,8,11,12b,13 |
| J1136.8−7413 | 174.0402 | −74.2626 | UNCL | 0.487 | - | 1 | 6 |
| J1137.9−1708 | 174.4808 | −17.1783 | BLLAC | - | - | - | |
| J1138.2+4115 | 174.5508 | 41.2311 | BLLAC | 0.315 | 0.142 | 3 | 1,11,13 |
| J1138.4+4857 | 174.5087 | 48.9826 | FSRQ | 0.878 | 0.162 | 4 | 1,3,12b,13 |
| J1139.0+4033 | 174.7614 | 40.5486 | FSRQ | 1.771 | 0.869 | 3 | 1,3,13 |
| J1139.0+5530 | 174.7533 | 55.5097 | UNCL | 0.628 | 0.222 | 3 | 1,3,13 |
| J1140.5+1528 | 175.0978 | 15.4694 | BLLAC | 0.142 | 0.055 | 7 | 5,6,7,8,11,12b,13 |
| J1141.4+6805 | 175.3272 | 68.0750 | UNCL | 0.599 | 0.159 | 5 | 4,7,8,12b,13 |
| J1141.5−1408 | 175.4242 | −14.1319 | BLLAC | 0.360 | 0.162 | 3 | 3,4,6 |
| J1142.0+1548 | 175.5322 | 15.7984 | BLLAC | 0.734 | 0.315 | 3 | 1,3,13 |
| J1143.1+6122 | 175.8004 | 61.3697 | BLLAC | 0.322 | 0.231 | 3 | 3,6,13 |
| J1144.9+1937 | 176.2709 | 19.6063 | MIS | 0.026 | 0.018 | 7 | 5,6,8,10,11,12b,13 |
| J1145.5+4423 | 176.4105 | 44.3394 | SEY | 0.226 | 0.087 | 8 | 3,4,6,7,8,11,12b,13 |
| J1145.5−0340 | 176.3963 | −3.6671 | BLLAC | 0.160 | 0.031 | 7 | 5,6,7,8,11,12b,13 |
| J1145.6+5552 | 176.3828 | 55.8802 | UNCL | 1.106 | - | 1 | 13 |
| J1145.7+0453 | 176.3388 | 4.9241 | FSRQ | 1.011 | 0.358 | 3 | 1,3,13 |
| J1146.4−3327 | 176.6185 | −33.4785 | FSRQ | 0.229 | - | 1 | 6 |
| J1146.6−2902 | 176.6091 | −28.9885 | BLLAC | 1.061 | - | 1 | 3 |
| J1146.9+3958 | 176.7429 | 39.9762 | FSRQ | 0.826 | 0.419 | 3 | 1,3,13 |
| J1147.0−3812 | 176.7557 | −38.2031 | BLLAC | - | - | - | |
| J1147.2−2627 | 176.7762 | −26.4207 | UNCL | 0.963 | - | 1 | 3 |
| J1147.8−0724 | 176.9648 | −7.4114 | FSRQ | 0.576 | 0.561 | 3 | 3,6,13 |
| J1148.5+2629 | 176.9990 | 26.5951 | FSRQ | 0.621 | 0.428 | 3 | 1,3,13 |
| J1148.6+1841 | 177.1574 | 18.6692 | BLLAC | 0.654 | 0.201 | 3 | 1,3,13 |
| J1149.0+5924 | 177.2098 | 59.4157 | MIS | 0.030 | 0.035 | 5 | 5,6,10,11,13 |
| J1149.1+2819 | 177.2871 | 28.4097 | UNCL | 1.238 | 0.897 | 4 | 1,3,4,13 |
| J1149.2+6246 | 177.3589 | 62.7257 | BLLAC | 0.478 | 0.225 | 3 | 1,3,13 |
| J1149.4+2441 | 177.3765 | 24.6575 | BLLAC | 0.254 | 0.114 | 4 | 1,6,12b,13 |
| J1149.5−4029 | 177.3238 | −40.4967 | UNCL | - | - | - | |
| J1150.4+2418 | 177.5801 | 24.2983 | BLLAC | 0.287 | 0.245 | 3 | 3,4,13 |
| J1150.6+4154 | 177.6448 | 41.9111 | BLLAC | 0.519 | 0.556 | 2 | 3,13 |
| J1150.6−4823 | 177.9077 | −48.3683 | UNCL | - | - | - | |
| J1151.3+0957 | 177.8221 | 9.9740 | BLLAC | 0.609 | 0.107 | 3 | 1,3,13 |
| J1151.5+5859 | 177.8528 | 58.9882 | BLLAC | 0.702 | 0.803 | 2 | 3,13 |
| J1151.5−1347 | 177.8749 | −13.7975 | BLLAC | 0.636 | 0.274 | 2 | 3,6 |
| J1151.6−2115 | 177.9180 | −21.2285 | UNCL | 0.700 | 0.315 | 3 | 3,4,6 |
| J1152.1+2837 | 178.0446 | 28.6225 | BLLAC | 0.214 | 0.067 | 6 | 6,7,8,11,12b,13 |
| J1152.3−0839 | 178.0717 | −8.6843 | FSRQ | 0.902 | 0.240 | 2 | 3,13 |
| J1152.8+3308 | 178.2163 | 33.1219 | FSRQ | 0.740 | 0.914 | 2 | 3,13 |
| J1153.0+8056 | 178.3021 | 80.9748 | FSRQ | 0.706 | 0.755 | 2 | 3,13 |
| J1153.3−1104 | 178.3430 | −11.0868 | FSRQ | 1.610 | - | 1 | 3 |
| J1153.4+4931 | 178.3519 | 49.5191 | FSRQ | 0.283 | 0.198 | 4 | 3,5,6,13 |
| J1153.6−2553 | 178.4102 | −25.9037 | UNCL | 0.683 | 0.154 | 3 | 3,4,6 |
| J1153.7+3822 | 178.4288 | 38.3850 | SEY | 0.319 | 0.098 | 5 | 1,3,6,12b,13 |
| J1154.0+4037 | 178.4777 | 40.6146 | NLS1 | 0.880 | 0.154 | 3 | 1,3,13 |
| J1154.0+6018 | 178.5189 | 60.3724 | FSRQ | 1.015 | 0.107 | 3 | 1,3,13 |
| J1154.0−0010 | 178.5190 | −0.1694 | BLLAC | 0.201 | 0.023 | 3 | 6,12b,13 |
| J1154.1−3243 | 178.5257 | −32.7119 | UNCL | 0.437 | - | 1 | 6 |
| J1155.5−3418 | 178.8355 | −34.2889 | BLLAC | 0.329 | - | 1 | 6 |
| J1155.8+6137 | 178.9517 | 61.5983 | BLLAC | 0.992 | 0.926 | 3 | 1,3,13 |
| J1156.6+0640 | 179.2527 | 6.6868 | UNCL | 1.156 | 0.271 | 4 | 1,3,4,13 |
| J1156.6−2248 | 179.1385 | −22.8346 | UNCL | 0.890 | 0.777 | 2 | 3,6 |
| J1158.5+4824 | 179.6115 | 48.4212 | FSRQ | 0.919 | 0.498 | 3 | 1,3,13 |
| J1158.9+0818 | 179.7217 | 8.3287 | AMB | 0.183 | 0.043 | 5 | 6,7,8,12b,13 |
| J1159.0+0939 | 179.7266 | 9.6199 | BLLAC | 0.873 | 0.668 | 3 | 1,3,13 |
| J1159.2−2227 | 179.7969 | −22.4769 | FSRQ | 0.770 | - | 1 | 3 |
| J1159.3−2142 | 179.8393 | −21.7125 | FSRQ | 1.105 | - | 1 | 3 |
| J1159.5+2914 | 179.8826 | 29.2455 | FSRQ | 0.409 | 0.202 | 3 | 1,3,13 |
| J1159.5−0723 | 179.8828 | −7.3999 | UNCL | 0.368 | 0.218 | 3 | 3,6,13 |
| J1200.2+0201 | 180.0515 | 2.0357 | UNCL | 0.635 | 0.451 | 5 | 6,7,8,12c,13 |
| J1200.6+1229 | 180.1668 | 12.5176 | BLLAC | 0.656 | 0.164 | 3 | 1,3,13 |
| J1200.7+2008 | 180.2380 | 20.1457 | UNCL | 0.430 | 0.308 | 3 | 11,12b,13 |
| J1200.8−1429 | 180.2297 | −14.5112 | UNCL | 0.698 | 0.277 | 3 | 3,4,6 |
| J1201.1−0332 | 180.2964 | −3.5388 | AMB | 0.683 | 0.095 | 4 | 1,3,12b,13 |
| J1201.7+1429 | 180.4345 | 14.5268 | BLLAC | 0.601 | 0.194 | 3 | 1,3,13 |
| J1202.4+4442 | 180.5361 | 44.7396 | BLLAC | 0.207 | 0.053 | 6 | 3,6,7,8,12b,13 |
| J1202.5+3852 | 180.7378 | 38.8632 | BLLAC | 0.771 | 0.543 | 3 | 1,3,13 |
| J1202.5−0528 | 180.6426 | −5.4674 | NLS1 | 0.290 | 0.252 | 2 | 3,13 |
| J1202.9+5141 | 180.7796 | 51.6752 | MIS | 0.064 | 0.014 | 8 | 5,6,7,8,10,11,12b,13 |
| J1203.1+6031 | 180.7646 | 60.5220 | SEY | 0.079 | 0.087 | 6 | 3,5,6,11,12b,13 |
| J1203.3+1119 | 180.8041 | 11.3048 | FSRQ | 0.953 | 0.182 | 4 | 1,3,4,13 |
| J1203.4−3925 | 180.8245 | −39.4392 | BLLAC | 0.185 | - | 1 | 6 |
| J1204.0+1146 | 181.0505 | 11.7654 | BLLAC | 0.165 | 0.104 | 4 | 7,8,12b,13 |
| J1204.2−0709 | 181.0694 | −7.1692 | BLLAC | 0.087 | 0.030 | 4 | 5,6,11,13 |
| J1204.8+0407 | 181.2153 | 4.1372 | FSRQ | 0.755 | 0.239 | 5 | 1,3,6,12c,13 |
| J1205.7−2635 | 181.3884 | −26.5679 | FSRQ | 0.718 | - | 1 | 3 |
| J1205.8+3321 | 181.4284 | 33.3631 | FSRQ | 0.427 | 0.329 | 2 | 6,13 |
| J1207.2−0524 | 181.8437 | −5.4117 | UNCL | - | - | - | |
| J1207.7−0106 | 181.9237 | −1.1102 | FSRQ | 0.772 | 0.543 | 3 | 1,3,13 |
| J1207.7−2229 | 181.9044 | −22.5099 | BLLAC | 0.760 | 0.649 | 2 | 3,6 |
| J1208.1+3017 | 182.0180 | 30.2640 | BLLAC | 0.618 | 0.330 | 3 | 3,4,13 |
| J1208.2−7810 | 182.0765 | −78.1635 | UNCL | - | - | - | |
| J1208.4+6121 | 182.1547 | 61.3518 | MIS | 0.209 | 0.065 | 7 | 3,6,7,8,11,12b,13 |
| J1208.9+5441 | 182.2261 | 54.6995 | NLS1 | 0.986 | 0.235 | 3 | 1,3,13 |
| J1209.0−4630 | 182.2716 | −46.4968 | UNCL | - | - | - | |
| J1209.4+4118 | 182.3449 | 41.3282 | BLLAC | 0.505 | 0.542 | 2 | 3,13 |
| J1209.4+7608 | 182.3762 | 76.1533 | UNCL | 0.486 | 0.307 | 4 | 3,4,6,13 |
| J1209.7+2548 | 182.4379 | 25.7844 | FSRQ | 1.150 | 0.365 | 3 | 1,3,13 |
| J1209.8+1810 | 182.4657 | 18.1686 | FSRQ | 0.709 | 0.147 | 3 | 1,3,13 |
| J1211.0−3800 | 182.7573 | −37.9219 | UNCL | - | - | - | |
| J1211.6+3901 | 182.8927 | 39.0149 | BLLAC | 0.668 | 0.100 | 4 | 7,8,12b,13 |
| J1211.6−2735 | 182.8992 | −27.6044 | UNCL | 0.760 | 0.081 | 2 | 3,4 |
| J1212.0+2242 | 182.9945 | 22.7090 | BLLAC | 0.310 | 0.095 | 3 | 1,12b,13 |
| J1212.0−2326 | 183.0189 | −23.4617 | BLLAC | 0.666 | 0.045 | 2 | 3,4 |
| J1212.7−1402 | 183.1695 | −14.0288 | UNCL | 0.244 | - | 1 | 6 |
| J1213.0+5129 | 183.2534 | 51.4932 | BLLAC | 0.555 | 0.434 | 3 | 1,3,13 |
| J1213.3−2618 | 183.3464 | −26.3022 | BLLAC | 0.170 | - | 1 | 6 |
| J1213.6+1306 | 183.3840 | 13.1225 | FSRQ | 0.802 | 0.499 | 3 | 1,3,13 |
| J1213.7+6423 | 183.4534 | 64.4222 | BLLAC | 0.734 | 0.221 | 3 | 1,3,13 |
| J1213.8−4345 | 183.4600 | −43.7235 | UNCL | - | - | - | |
| J1214.6−1926 | 183.5154 | −19.3619 | NLS1 | 0.132 | - | 1 | 5 |
| J1215.0+1656 | 183.7666 | 16.9105 | FSRQ | 0.739 | 0.670 | 2 | 3,13 |
| J1215.1+0731 | 183.7957 | 7.5346 | BLLAC | 0.081 | 0.016 | 4 | 10,11,12b,13 |
| J1215.1+3513 | 183.7869 | 35.1371 | BLLAC | 0.504 | 0.156 | 5 | 6,7,8,12b,13 |
| J1215.1+5002 | 183.7533 | 50.0376 | BLLAC | 0.622 | 0.719 | 2 | 3,13 |
| J1215.8−1733 | 183.9448 | −17.5293 | UNCL | - | - | - | |
| J1215.8−3732 | 184.0084 | −37.5703 | UNCL | - | - | - | |
| J1216.1+0930 | 184.0259 | 9.4860 | SEY | 0.075 | 0.014 | 5 | 5,6,10,12b,13 |
| J1216.1−0242 | 184.0136 | −2.7183 | BLLAC | 0.219 | 0.064 | 2 | 6,13 |
| J1217.9+3007 | 184.4670 | 30.1168 | BLLAC | 0.115 | 0.078 | 3 | 3,6,13 |
| J1218.0−0028 | 184.4947 | −0.4962 | BLLAC | 0.436 | 0.176 | 4 | 3,6,8,13 |
| J1218.5−0119 | 184.6455 | −1.3318 | BLLAC | 0.498 | 0.635 | 2 | 3,13 |
| J1219.0+4827 | 184.7767 | 48.4989 | FSRQ | 0.802 | 0.307 | 4 | 1,3,6,13 |
| J1219.0−4827 | 184.7594 | −48.4411 | BLLAC | 0.200 | - | 1 | 4 |
| J1219.6+0550 | 184.8467 | 5.8249 | MIS | 0.009 | 0.003 | 4 | 5,6,12b,13 |
| J1219.7+0444 | 184.9374 | 4.7729 | BLLAC | 0.138 | - | 1 | 13 |
| J1219.7−0313 | 184.9405 | −3.2400 | BLLAC | 0.282 | 0.263 | 3 | 3,8,13 |
| J1219.9+6056 | 184.9109 | 60.9656 | UNCL | 0.851 | 0.024 | 3 | 11,12b,13 |
| J1220.1+3432 | 185.0346 | 34.5227 | BLLAC | 0.489 | 0.513 | 2 | 3,13 |
| J1220.1+7105 | 185.0151 | 71.0920 | AMB | 0.649 | 0.804 | 2 | 3,13 |
| J1220.2−3713 | 185.0825 | −37.2373 | UNCL | 0.300 | - | 1 | 4 |
| J1221.3+3010 | 185.3414 | 30.1770 | BLLAC | 0.203 | 0.184 | 4 | 3,5,6,13 |
| J1221.5+2814 | 185.3820 | 28.2329 | BLLAC | 0.229 | 0.220 | 3 | 3,6,13 |
| J1222.0−4121 | 185.5423 | −41.3826 | UNCL | - | - | - | |
| J1222.5+0414 | 185.5940 | 4.2210 | FSRQ | 0.388 | 0.462 | 2 | 3,13 |
| J1223.0+1100 | 185.7802 | 11.0106 | BLLAC | 1.148 | 0.783 | 3 | 1,3,13 |
| J1223.3+1213 | 185.8683 | 12.1257 | UNCL | 0.998 | 0.173 | 3 | 11,12b,13 |
| J1223.6−3032 | 185.9042 | −30.5473 | BLLAC | 0.201 | 0.082 | 3 | 4,6,11 |
| J1223.8+4649 | 185.9712 | 46.8467 | BLLAC | 0.228 | 0.030 | 6 | 6,7,8,11,12b,13 |
| J1223.8+8039 | 185.9187 | 80.6679 | BLLAC | 0.469 | 0.368 | 3 | 3,6,13 |
| J1223.9+5000 | 186.0413 | 50.0321 | FSRQ | 0.487 | 0.508 | 3 | 3,6,13 |
| J1223.9+7954 | 185.9920 | 79.8912 | BLLAC | 0.208 | 0.060 | 4 | 6,11,12b,13 |
| J1224.1+2239 | 186.0043 | 22.6610 | BLLAC | 0.479 | 0.151 | 4 | 1,3,6,13 |
| J1224.4+2436 | 186.1008 | 24.6065 | BLLAC | 0.839 | 0.940 | 2 | 3,13 |
| J1224.7−8313 | 186.2266 | −83.2195 | UNCL | - | - | - | |
| J1224.9+2122 | 186.2269 | 21.3796 | FSRQ | 0.444 | 0.544 | 2 | 3,13 |
| J1224.9+4334 | 186.2146 | 43.5887 | AMB | 0.772 | 0.283 | 3 | 1,3,13 |
| J1225.0+0330 | 186.2184 | 3.5140 | FSRQ | 0.655 | 0.393 | 3 | 1,3,13 |
| J1225.3−3446 | 186.4034 | −34.7894 | BLLAC | 0.260 | 0.053 | 2 | 4,6 |
| J1225.4−1550 | 186.3554 | −15.8881 | UNCL | 0.272 | 0.038 | 2 | 4,6 |
| J1225.5−2851 | 186.3146 | −28.8315 | UNCL | 1.723 | - | 1 | 3 |
| J1225.6−7313 | 186.3970 | −73.2277 | UNCL | 0.294 | - | 1 | 6 |
| J1226.7+0637 | 186.6843 | 6.6481 | BLLAC | 0.163 | - | 1 | 13 |
| J1226.8−1329 | 186.7267 | −13.4775 | BLLAC | 1.301 | - | 1 | 3 |
| J1227.1−4437 | 186.8612 | −44.6107 | BLLAC | - | - | - | |
| J1228.7+4858 | 187.2157 | 48.9670 | FSRQ | 1.178 | 0.621 | 3 | 1,3,13 |
| J1229.0+0202 | 187.2779 | 2.0524 | FSRQ | 0.054 | 0.021 | 4 | 5,6,11,13 |
| J1230.2+2517 | 187.5587 | 25.3020 | BLLAC | 0.555 | 0.672 | 2 | 3,13 |
| J1230.8+1223 | 187.7059 | 12.3911 | MIS | 0.040 | 0.058 | 4 | 5,6,12b,13 |
| J1230.9+3711 | 187.8504 | 37.1839 | MIS | 0.204 | 0.030 | 6 | 6,7,8,11,12b,13 |
| J1231.5+1421 | 187.8496 | 14.3568 | BLLAC | 0.109 | 0.024 | 4 | 5,6,11,13 |
| J1231.6+6415 | 187.8808 | 64.2384 | BLLAC | 0.114 | 0.025 | 6 | 5,6,10,11,12b,13 |
| J1231.7+2847 | 187.9316 | 28.7972 | BLLAC | 0.344 | 0.308 | 3 | 3,6,13 |
| J1232.5+4821 | 188.1449 | 48.3592 | FSRQ | 0.593 | 0.384 | 4 | 3,7,8,13 |
| J1232.5−3720 | 188.1500 | −37.3476 | UNCL | - | - | - | |
| J1233.1+1703 | 188.2714 | 17.0259 | BLLAC | 0.719 | 0.818 | 2 | 3,13 |
| J1233.6+5027 | 188.4553 | 50.4397 | AMB | 0.154 | 0.042 | 7 | 3,6,7,8,11,12b,13 |
| J1233.7−0144 | 188.4222 | −1.7399 | BLLAC | 0.581 | 0.424 | 3 | 1,3,13 |
| J1234.7−0434 | 188.6842 | −4.6062 | UNCL | 0.629 | 0.059 | 2 | 3,13 |
| J1236.3+3858 | 189.0959 | 39.0003 | BLLAC | 0.208 | 0.062 | 5 | 6,7,8,12b,13 |
| J1237.0+3019 | 189.2733 | 30.3348 | BLLAC | 0.770 | 0.407 | 4 | 1,3,4,13 |
| J1237.8+6256 | 189.4128 | 62.9786 | BLLAC | 0.188 | 0.049 | 5 | 6,7,8,12b,13 |
| J1238.1−4541 | 189.5251 | −45.6916 | BLLAC | 0.362 | 0.185 | 2 | 4,6 |
| J1238.3−1959 | 189.6016 | −19.9871 | BLLAC | 0.704 | 0.665 | 2 | 3,6 |
| J1238.5−1201 | 189.5309 | −11.9902 | FSRQ | 0.224 | - | 1 | 3 |
| J1239.4+0728 | 189.8525 | 7.5048 | BLLAC | 0.552 | 0.604 | 2 | 3,13 |
| J1239.5+0443 | 189.8865 | 4.7181 | FSRQ | 0.705 | 0.097 | 3 | 1,3,13 |
| J1240.4−2606 | 190.1209 | −26.1553 | UNCL | 1.184 | - | 1 | 3 |
| J1241.3+4236 | 190.3751 | 42.6606 | BLLAC | 0.556 | 0.175 | 5 | 3,7,8,12b,13 |
| J1241.5+3439 | 190.4217 | 34.6756 | BLLAC | 0.266 | - | 1 | 6 |
| J1241.8−1456 | 190.4557 | −14.9329 | BLLAC | 0.134 | - | 1 | 6 |
| J1241.9+0636 | 190.4512 | 6.6003 | BLLAC | 1.566 | 0.744 | 3 | 1,3,13 |
| J1242.6+7635 | 190.6346 | 76.5716 | UNCL | 0.485 | 0.020 | 2 | 4,13 |
| J1242.9+7315 | 190.7967 | 73.2665 | BLLAC | 0.062 | 0.007 | 5 | 5,6,11,12b,13 |
| J1243.0+3950 | 190.8288 | 39.8549 | AMB | 1.061 | 0.282 | 3 | 1,3,13 |
| J1243.2+3627 | 190.8031 | 36.4622 | BLLAC | 0.036 | - | 1 | 13 |
| J1243.9−0218 | 190.9687 | −2.3107 | BLLAC | 0.788 | 0.041 | 4 | 11,12b,12c,13 |
| J1244.2−4956 | 191.0957 | −49.9062 | UNCL | 0.301 | 0.141 | 3 | 4,5,6 |
| J1244.5+1616 | 191.1848 | 16.2727 | BLLAC | 0.359 | 0.052 | 6 | 6,7,8,11,12b,13 |
| J1245.1+5709 | 191.2917 | 57.1651 | BLLAC | 0.542 | 0.588 | 2 | 3,13 |
| J1245.8+0232 | 191.3908 | 2.4737 | BLLAC | 0.710 | 0.333 | 3 | 1,3,13 |
| J1246.3+0112 | 191.5106 | 1.2219 | BLLAC | 0.552 | 0.657 | 8 | 1,3,6,8,11,12b,12c,13 |
| J1246.7−2548 | 191.6950 | −25.7970 | NLS1 | 0.387 | 0.221 | 2 | 3,6 |
| J1247.0+4421 | 191.7530 | 44.3888 | BLLAC | 0.272 | 0.240 | 2 | 1,13 |
| J1248.3+5820 | 192.0783 | 58.3413 | BLLAC | 0.508 | 0.631 | 2 | 3,13 |
| J1248.7+5127 | 192.1429 | 51.4689 | BLLAC | 0.275 | 0.111 | 3 | 3,12b,13 |
| J1248.9+4840 | 192.2123 | 48.6648 | FSRQ | 1.421 | 0.472 | 3 | 1,3,13 |
| J1249.2−2809 | 192.3305 | −28.1429 | UNCL | 0.103 | 0.058 | 4 | 4,5,6,11 |
| J1249.3−0545 | 192.3307 | −5.7610 | UNCL | 0.223 | 0.033 | 6 | 6,7,8,11,12b,13 |
| J1249.8+3707 | 192.4448 | 37.1300 | BLLAC | 0.883 | 0.555 | 3 | 1,3,13 |
| J1250.6+0217 | 192.6358 | 2.2756 | BLLAC | 0.731 | 0.282 | 3 | 1,3,13 |
| J1250.8+3117 | 192.7160 | 31.2850 | UNCL | 0.304 | 0.057 | 7 | 4,6,7,8,11,12b,13 |
| J1251.2+1039 | 192.8245 | 10.6520 | BLLAC | 0.241 | 0.108 | 6 | 3,6,7,8,12b,13 |
| J1251.3−0201 | 192.8266 | −2.0354 | UNCL | 0.414 | 0.360 | 3 | 3,4,13 |
| J1251.3−1719 | 192.8103 | −17.2870 | FSRQ | 0.727 | 0.304 | 2 | 3,6 |
| J1253.2+5301 | 193.2997 | 53.0199 | BLLAC | 0.721 | 0.908 | 2 | 3,13 |
| J1253.5−3934 | 193.4212 | −39.5331 | BLLAC | 0.163 | 0.018 | 2 | 5,6 |
| J1253.8+0327 | 193.4459 | 3.4418 | BLLAC | 0.040 | 0.006 | 8 | 5,6,7,8,10,11,12b,13 |
| J1253.8+6242 | 193.4971 | 62.7160 | BLLAC | 0.515 | 0.418 | 3 | 1,3,13 |
| J1254.2−2205 | 193.5936 | −22.0705 | UNCL | 0.700 | - | 1 | 4 |
| J1254.5+2210 | 193.6386 | 22.1843 | BLLAC | 0.525 | 0.526 | 3 | 3,6,13 |
| J1254.9+1138 | 193.6594 | 11.6850 | FSRQ | 0.492 | 0.598 | 2 | 3,13 |
| J1254.9−4426 | 193.7396 | −44.4157 | BLLAC | 0.028 | 0.007 | 2 | 5,6 |
| J1256.1−0547 | 194.0465 | −5.7893 | FSRQ | 0.026 | - | 1 | 13 |
| J1256.2−1146 | 194.0665 | −11.7770 | BLLAC | 0.035 | 0.005 | 3 | 5,6,11 |
| J1257.2+3646 | 194.3191 | 36.7875 | BLLAC | 0.403 | 0.310 | 3 | 3,6,13 |
| J1257.6+2413 | 194.3830 | 24.2111 | BLLAC | 0.133 | 0.036 | 7 | 5,6,7,8,11,12b,13 |
| J1257.8+3228 | 194.4885 | 32.4915 | FSRQ | 0.636 | 0.417 | 3 | 1,3,13 |
| J1258.3+6121 | 194.5866 | 61.3460 | BLLAC | 0.204 | 0.046 | 5 | 6,7,8,12b,13 |
| J1258.6−1759 | 194.6596 | −18.0009 | FSRQ | 0.852 | 0.402 | 2 | 3,6 |
| J1258.7+5143 | 194.6058 | 51.7073 | UNCL | 0.441 | 0.174 | 7 | 3,4,6,7,8,12b,13 |
| J1258.7−0452 | 194.7002 | −4.7959 | BLLAC | 0.113 | - | 1 | 13 |
| J1258.8−2219 | 194.7270 | −22.3253 | FSRQ | 1.205 | 0.041 | 2 | 1,3 |
| J1259.1−2311 | 194.7853 | −23.1774 | FSRQ | 0.382 | 0.319 | 2 | 3,6 |
| J1259.5+2332 | 194.9012 | 23.5131 | UNCL | 0.237 | 0.069 | 8 | 3,4,6,7,8,11,12b,13 |
| J1259.7−3223 | 194.9576 | −32.3914 | BLLAC | - | - | - | |
| J1259.8−3749 | 194.9575 | −37.8162 | BLLAC | 0.224 | 0.031 | 2 | 4,6 |
| J1300.0+1753 | 195.0355 | 17.9271 | BLLAC | 0.835 | 0.605 | 4 | 1,3,4,13 |
| J1300.4+1416 | 195.0872 | 14.2885 | FSRQ | 0.782 | 0.526 | 3 | 1,3,13 |
| J1301.5+4413 | 195.4430 | 44.2720 | BLLAC | 0.520 | 0.316 | 3 | 1,3,13 |
| J1301.6+3336 | 195.3715 | 33.6168 | FSRQ | 0.954 | 0.373 | 3 | 1,3,13 |
| J1301.6+4056 | 195.4402 | 40.9402 | BLLAC | 0.572 | 0.479 | 3 | 1,3,13 |
| J1302.3+6901 | 195.6580 | 69.0477 | AMB | 0.571 | 0.144 | 4 | 3,6,12b,13 |
| J1302.7+4750 | 195.7029 | 47.9196 | BLLAC | 0.124 | 0.014 | 8 | 5,6,7,8,10,11,12b,13 |
| J1302.8+5748 | 195.7186 | 57.8104 | CLAGN | 1.320 | 0.574 | 3 | 1,3,13 |
| J1303.0+2434 | 195.7634 | 24.5655 | BLLAC | 0.806 | 0.701 | 4 | 1,3,11,13 |
| J1303.6−4622 | 195.9178 | −46.3507 | FSRQ | - | - | - | |
| J1304.0+3704 | 196.0305 | 37.1523 | BLLAC | 0.392 | 0.184 | 3 | 1,3,13 |
| J1304.2−2412 | 196.0696 | −24.2047 | UNCL | 1.264 | - | 1 | 3 |
| J1304.3−4353 | 196.0875 | −43.8862 | BLLAC | - | - | - | |
| J1304.6−0348 | 196.1818 | −3.7674 | FSRQ | 1.034 | 0.350 | 2 | 3,13 |
| J1304.9−2107 | 196.2461 | −21.1118 | UNCL | 0.938 | - | 1 | 3 |
| J1305.3+5118 | 196.3448 | 51.2778 | NLS1 | 0.576 | 0.409 | 2 | 3,13 |
| J1305.6+7853 | 196.2501 | 78.9099 | UNCL | 0.610 | 0.136 | 3 | 3,6,13 |
| J1305.9+3858 | 196.3800 | 38.9225 | MIS | 0.282 | 0.051 | 6 | 6,7,8,11,12b,13 |
| J1306.3+1113 | 196.5802 | 11.2277 | MIS | 0.079 | 0.016 | 8 | 5,6,7,8,10,11,12b,13 |
| J1306.7−2148 | 196.6752 | −21.7975 | MIS | 0.142 | 0.053 | 6 | 3,5,6,7,8,11 |
| J1307.6−4259 | 196.9083 | −42.9942 | BLLAC | - | - | - | |
| J1308.5+3547 | 197.0988 | 35.7770 | FSRQ | 0.997 | 0.533 | 4 | 1,3,6,13 |
| J1309.4+4305 | 197.3564 | 43.0849 | BLLAC | 0.683 | 0.757 | 2 | 3,13 |
| J1309.7+1153 | 197.3914 | 11.9068 | BLLAC | 0.659 | 0.220 | 3 | 1,3,13 |
| J1310.2−1158 | 197.5519 | −11.9630 | BLLAC | 0.083 | 0.015 | 3 | 5,6,11 |
| J1310.5+3221 | 197.6194 | 32.3455 | FSRQ | 0.881 | 0.296 | 2 | 3,13 |
| J1310.6+2449 | 197.6605 | 24.8062 | BLLAC | 0.207 | 0.034 | 6 | 6,7,8,11,12b,13 |
| J1310.9+5514 | 197.7634 | 55.2318 | NLS1 | 0.530 | 0.324 | 3 | 1,3,13 |
| J1311.0+0034 | 197.7770 | 0.5861 | BLLAC | 0.384 | 0.401 | 4 | 3,6,8,13 |
| J1311.0+3233 | 197.7475 | 32.5596 | FSRQ | 1.264 | 0.523 | 3 | 1,3,13 |
| J1311.8+2057 | 197.9310 | 20.8690 | MIS | 0.724 | 0.224 | 4 | 1,3,4,13 |
| J1311.8+3954 | 197.9421 | 39.8881 | BLLAC | 0.550 | 0.164 | 3 | 1,3,13 |
| J1312.4−2156 | 198.1315 | −21.9398 | BLLAC | 0.375 | 0.281 | 2 | 3,6 |
| J1312.6+4828 | 198.1806 | 48.4753 | AMB | 0.522 | 0.111 | 6 | 6,7,8,11,12b,13 |
| J1312.6−1900 | 198.1446 | −18.9837 | UNCL | 0.391 | 0.145 | 2 | 4,6 |
| J1312.8−0425 | 198.2121 | −4.4139 | FSRQ | 0.724 | - | 1 | 13 |
| J1312.8−2350 | 198.2032 | −23.8464 | BLLAC | 1.261 | - | 1 | 3 |
| J1314.7+2348 | 198.6825 | 23.8074 | BLLAC | 0.485 | 0.432 | 2 | 3,13 |
| J1315.0−4236 | 198.7642 | −42.6139 | BLLAC | 0.112 | 0.003 | 2 | 5,6 |
| J1315.4+8453 | 200.2216 | 84.8364 | UNCL | 0.573 | - | 1 | 11 |
| J1315.5+1135 | 198.8859 | 11.5588 | BLLAC | 0.406 | 0.022 | 3 | 1,4,13 |
| J1315.9−0732 | 198.9707 | −7.5506 | BLLAC | 0.200 | 0.093 | 2 | 6,13 |
| J1316.1−3338 | 199.0333 | −33.6498 | FSRQ | - | - | - | |
| J1316.5+3013 | 199.2274 | 30.2484 | BLLAC | 0.586 | 0.304 | 3 | 1,3,13 |
| J1317.1+6613 | 199.4716 | 66.2654 | UNCL | 0.920 | 0.522 | 2 | 3,13 |
| J1317.6+3428 | 199.4021 | 34.4211 | FSRQ | 0.690 | 0.439 | 3 | 1,3,13 |
| J1317.6+7450 | 199.5955 | 74.8098 | UNCL | 0.895 | 0.728 | 3 | 3,4,13 |
| J1318.1−1740 | 199.5339 | −17.5935 | UNCL | 0.622 | 0.296 | 2 | 3,4 |
| J1318.2+6754 | 199.6679 | 67.9067 | UNCL | 0.977 | 0.401 | 4 | 1,3,4,13 |
| J1318.7−1234 | 199.6786 | −12.5844 | UNCL | 1.178 | - | 1 | 3 |
| J1319.5+1404 | 199.8823 | 14.0925 | BLLAC | 0.394 | 0.288 | 3 | 3,6,13 |
| J1319.5−0045 | 199.9115 | −0.8278 | MIS | 1.088 | 1.403 | 2 | 3,13 |
| J1319.8+7759 | 199.8386 | 77.9729 | UNCL | 0.156 | 0.047 | 3 | 4,6,13 |
| J1321.1+2216 | 200.2967 | 22.2700 | NLS1 | 0.883 | 0.267 | 3 | 1,3,13 |
| J1321.3−2641 | 200.3085 | −26.6029 | FSRQ | 1.065 | - | 1 | 3 |
| J1321.9+3219 | 200.5004 | 32.3175 | BLLAC | 0.381 | 0.027 | 7 | 6,7,8,10,11,12b,13 |
| J1322.0+8317 | 200.4400 | 83.2704 | UNCL | 0.934 | 0.283 | 4 | 3,11,12b,13 |
| J1322.2+0842 | 200.5424 | 8.7091 | CLAGN | 0.353 | 0.048 | 6 | 3,6,7,8,12b,13 |
| J1322.3−0606 | 200.5837 | −6.1049 | UNCL | 0.677 | 0.466 | 3 | 3,4,13 |
| J1322.6−0936 | 200.6538 | −9.6272 | FSRQ | 1.004 | 0.884 | 2 | 3,13 |
| J1322.6−1418 | 200.6274 | −14.3151 | UNCL | 0.659 | 0.093 | 3 | 3,4,6 |
| J1322.6−1617 | 200.6819 | −16.2902 | UNCL | 0.525 | 0.350 | 3 | 3,4,6 |
| J1322.9+0437 | 200.7542 | 4.6643 | BLLAC | 0.140 | 0.046 | 7 | 5,6,7,8,10,11,13 |
| J1323.0+2941 | 200.7536 | 29.6958 | FSRQ | 0.739 | 0.244 | 3 | 1,3,13 |
| J1323.9+1405 | 200.9932 | 14.0999 | BLLAC | 0.293 | 0.231 | 2 | 1,13 |
| J1324.9+4748 | 201.1223 | 47.7224 | FSRQ | 0.530 | 0.439 | 4 | 3,7,8,13 |
| J1325.5−4300 | 201.3651 | −43.0191 | MIS | - | - | - | |
| J1325.6−0227 | 201.4246 | −2.4694 | BLLAC | 0.459 | 0.190 | 5 | 1,3,6,8,13 |
| J1326.1+1232 | 201.5738 | 12.4997 | BLLAC | 0.161 | 0.037 | 7 | 5,6,7,8,11,12b,13 |
| J1326.7−0503 | 201.7276 | −5.0164 | FSRQ | 1.219 | 0.742 | 2 | 3,13 |
| J1326.9+2210 | 201.7536 | 22.1806 | FSRQ | 0.986 | 0.291 | 3 | 1,3,13 |
| J1327.8+2522 | 201.9956 | 25.4629 | BLLAC | 1.014 | 0.629 | 3 | 1,3,13 |
| J1328.5−4727 | 202.1693 | −47.4637 | BLLAC | 0.236 | - | 1 | 6 |
| J1328.6+1145 | 202.1398 | 11.7557 | BLLAC | 0.338 | 0.091 | 3 | 1,12b,13 |
| J1329.4−0530 | 202.3692 | −5.5267 | FSRQ | 0.360 | 0.453 | 2 | 3,13 |
| J1330.2+7002 | 202.6075 | 70.0274 | BLLAC | 0.343 | 0.314 | 3 | 3,4,13 |
| J1330.3+4441 | 202.5897 | 44.6890 | BLLAC | 0.439 | 0.002 | 2 | 1,13 |
| J1330.4+3157 | 202.4703 | 31.9031 | BLLAC | 0.731 | 0.345 | 3 | 1,3,13 |
| J1330.7+5200 | 202.6775 | 52.0376 | AMB | 0.668 | 0.089 | 5 | 7,8,11,12b,13 |
| J1331.0+3032 | 202.7845 | 30.5092 | MIS | 0.520 | 0.546 | 2 | 3,13 |
| J1331.0+5653 | 202.7621 | 56.9283 | BLLAC | 0.236 | 0.034 | 6 | 6,7,8,11,12b,13 |
| J1331.2−1325 | 202.8348 | −13.4349 | FSRQ | 0.537 | 0.201 | 2 | 3,6 |
| J1331.6+1711 | 202.8894 | 17.2141 | BLLAC | 0.631 | 0.308 | 3 | 1,3,13 |
| J1331.7−0343 | 202.8715 | −3.6873 | FSRQ | 1.034 | 0.685 | 2 | 3,13 |
| J1331.7−0647 | 202.9453 | −6.7759 | BLLAC | 0.382 | 0.451 | 5 | 3,4,6,11,13 |
| J1332.0−0509 | 203.0186 | −5.1620 | FSRQ | 0.494 | 0.390 | 3 | 3,6,13 |
| J1332.2+4722 | 203.1885 | 47.3730 | FSRQ | 0.522 | 0.595 | 2 | 3,13 |
| J1332.6−1256 | 203.1635 | −12.9376 | FSRQ | 1.047 | - | 1 | 3 |
| J1333.2+2725 | 203.2812 | 27.4218 | CLAGN | 0.851 | 0.189 | 4 | 1,3,6,13 |
| J1333.7+5056 | 203.4741 | 50.9600 | FSRQ | 1.144 | 1.323 | 2 | 1,13 |
| J1334.1−3521 | 203.5501 | −35.3372 | UNCL | - | - | - | |
| J1334.5+5634 | 203.6562 | 56.5300 | MIS | 0.465 | 0.282 | 4 | 1,3,12b,13 |
| J1335.3−2949 | 203.8740 | −29.8441 | BLLAC | 1.649 | - | 1 | 3 |
| J1336.2+2320 | 204.0507 | 23.3328 | BLLAC | 0.206 | 0.050 | 5 | 6,7,8,12b,13 |
| J1337.4+5502 | 204.4568 | 55.0173 | FSRQ | 0.842 | 0.445 | 4 | 1,3,4,13 |
| J1337.5−7802 | 204.5335 | −78.0168 | UNCL | - | - | - | |
| J1337.6−1257 | 204.4158 | −12.9569 | FSRQ | 0.718 | - | 1 | 3 |
| J1337.9−1956 | 204.4472 | −19.9699 | UNCL | 0.482 | 0.110 | 2 | 4,6 |
| J1338.0+6534 | 204.3169 | 65.5462 | FSRQ | 0.759 | 0.164 | 3 | 1,3,13 |
| J1338.9+1153 | 204.7461 | 11.8880 | BLLAC | 0.771 | 0.858 | 2 | 3,13 |
| J1339.0−2400 | 204.7573 | −24.0206 | FSRQ | 0.723 | 0.542 | 2 | 3,11 |
| J1339.1−2620 | 204.8329 | −26.3418 | FSRQ | 0.968 | - | 1 | 3 |
| J1339.9−0138 | 205.0192 | −1.6296 | FSRQ | 1.093 | 0.869 | 4 | 1,3,6,13 |
| J1340.1+3857 | 204.7070 | 38.8531 | MIS | - | - | - | |
| J1340.4+6926 | 205.2000 | 69.3896 | FSRQ | 1.460 | 0.942 | 2 | 3,13 |
| J1340.5+4409 | 205.1242 | 44.1678 | BLLAC | 0.237 | 0.129 | 5 | 6,7,8,12b,13 |
| J1340.8−0409 | 205.1751 | −4.1686 | BLLAC | 0.179 | 0.100 | 4 | 3,6,11,13 |
| J1341.1+7433 | 205.3273 | 74.5819 | UNCL | 0.761 | 0.322 | 3 | 3,6,13 |
| J1341.2+3958 | 205.2713 | 39.9959 | AMB | 0.124 | 0.042 | 7 | 5,6,7,8,11,12b,13 |
| J1341.6+5515 | 205.4008 | 55.2436 | BLLAC | 0.188 | 0.046 | 7 | 3,6,7,8,11,12b,13 |
| J1341.7−3907 | 205.4749 | −39.1166 | UNCL | 0.243 | 0.017 | 2 | 5,6 |
| J1341.8−2053 | 205.5197 | −20.8582 | FSRQ | 0.853 | 0.879 | 2 | 3,6 |
| J1342.6+0944 | 205.6668 | 9.7979 | BLLAC | 0.272 | 0.020 | 6 | 3,6,7,8,12b,13 |
| J1342.7+0505 | 205.6818 | 5.0756 | MIS | 0.100 | 0.020 | 8 | 5,6,7,8,10,11,12b,13 |
| J1343.6+5755 | 205.9901 | 57.9118 | FSRQ | 0.698 | 0.469 | 3 | 1,3,13 |
| J1344.0+6605 | 206.0362 | 66.1032 | FSRQ | 1.122 | 0.092 | 3 | 1,3,13 |
| J1344.1−7700 | 205.9653 | −76.9695 | UNCL | - | - | - | |
| J1344.2−1723 | 206.0600 | −17.3946 | FSRQ | 0.620 | - | 1 | 6 |
| J1344.4−3656 | 206.0991 | −36.9413 | UNCL | - | - | - | |
| J1345.5+4453 | 206.3882 | 44.8832 | FSRQ | 0.763 | 0.325 | 5 | 1,3,6,11,13 |
| J1345.6−3356 | 206.4294 | −33.9454 | UNCL | - | - | - | |
| J1345.8+0706 | 206.4555 | 7.1086 | FSRQ | 1.117 | 0.330 | 3 | 1,3,13 |
| J1347.1−2959 | 206.7787 | −29.9785 | BLLAC | - | - | - | |
| J1347.4+7309 | 206.8943 | 73.3036 | UNCL | 1.133 | 0.247 | 3 | 3,4,13 |
| J1347.6−3751 | 206.9185 | −37.8435 | FSRQ | 1.300 | - | 1 | 4 |
| J1348.9+0756 | 207.2225 | 7.9466 | BLLAC | 0.172 | 0.029 | 8 | 5,6,7,8,10,11,12b,13 |
| J1349.5−1131 | 207.3810 | −11.5483 | FSRQ | 0.507 | 0.402 | 2 | 3,6 |
| J1350.8+3033 | 207.7197 | 30.5816 | FSRQ | 0.796 | 0.304 | 2 | 3,13 |
| J1351.0+0029 | 207.7685 | 0.5221 | FSRQ | 0.652 | 0.367 | 2 | 11,13 |
| J1351.3+1115 | 207.8369 | 11.2481 | BLLAC | 0.456 | 0.444 | 4 | 1,4,6,13 |
| J1351.4−1529 | 207.8228 | −15.5044 | BLLAC | 0.213 | - | 1 | 6 |
| J1351.7+5542 | 207.9925 | 55.7030 | BLLAC | 1.163 | 1.012 | 2 | 1,13 |
| J1351.7−2912 | 207.9452 | −29.2049 | BLLAC | - | - | - | |
| J1352.7−2742 | 208.1169 | −27.7520 | UNCL | 1.303 | 0.538 | 2 | 3,4 |
| J1353.0−4413 | 208.2356 | −44.2112 | BLLAC | - | - | - | |
| J1353.2+3740 | 208.3087 | 37.6872 | BLLAC | 0.152 | 0.041 | 7 | 5,6,7,8,11,12b,13 |
| J1353.3+1434 | 208.3452 | 14.5942 | BLLAC | 0.752 | 0.338 | 3 | 1,3,13 |
| J1353.4+5600 | 208.3669 | 56.0158 | BLLAC | 0.296 | 0.108 | 5 | 1,3,6,12b,13 |
| J1353.7−3936 | 208.4381 | −39.6197 | BLLAC | 0.358 | 0.056 | 2 | 4,6 |
| J1354.2+6934 | 208.5129 | 69.5303 | UNCL | 1.034 | 0.122 | 3 | 3,12b,13 |
| J1354.3−0206 | 208.5287 | −2.1009 | FSRQ | 2.260 | 1.450 | 3 | 1,3,13 |
| J1354.4+3707 | 208.6112 | 37.1152 | BLLAC | 0.492 | 0.451 | 3 | 3,6,13 |
| J1354.7+0623 | 208.6842 | 6.3800 | BLLAC | 0.231 | 0.042 | 7 | 3,6,7,8,11,12b,13 |
| J1354.8−1041 | 208.6938 | −10.6841 | FSRQ | 1.224 | - | 1 | 3 |
| J1356.2−1726 | 209.0290 | −17.4088 | MIS | 0.056 | 0.001 | 3 | 5,6,11 |
| J1357.1+1921 | 209.2685 | 19.3187 | FSRQ | 0.464 | 0.581 | 2 | 3,13 |
| J1357.5+0127 | 209.4112 | 1.4705 | BLLAC | 0.246 | 0.197 | 3 | 3,8,13 |
| J1358.1+7642 | 209.4807 | 76.7225 | FSRQ | 1.044 | 0.146 | 3 | 3,12b,13 |
| J1358.9−0703 | 209.7108 | −7.0671 | UNCL | 0.855 | 0.650 | 5 | 1,3,4,6,13 |
| J1359.1+5544 | 209.7739 | 55.7415 | FSRQ | 0.633 | 0.465 | 3 | 1,3,13 |
| J1359.4+0202 | 209.8631 | 1.9985 | FSRQ | 0.887 | 0.602 | 3 | 1,3,13 |
| J1359.7+4012 | 209.9087 | 40.1940 | FSRQ | 0.242 | 0.082 | 6 | 3,6,7,8,12b,13 |
| J1359.8−3746 | 209.9572 | −37.7669 | BLLAC | - | - | - | |
| J1400.2−4010 | 210.0920 | −40.1399 | BLLAC | 0.194 | - | 1 | 6 |
| J1401.1−3717 | 210.3084 | −37.2996 | UNCL | - | - | - | |
| J1401.2−0915 | 210.2722 | −9.2754 | FSRQ | 0.973 | 0.399 | 2 | 1,3 |
| J1402.5−1827 | 210.6906 | −18.4323 | UNCL | 1.004 | 0.775 | 3 | 3,4,6 |
| J1402.6+1600 | 210.6855 | 15.9991 | AMB | 0.198 | 0.094 | 6 | 3,5,6,11,12b,13 |
| J1402.6−3330 | 210.6725 | −33.5692 | FSRQ | - | - | - | |
| J1404.8+0402 | 211.2121 | 4.0339 | BLLAC | 0.920 | 1.189 | 2 | 3,13 |
| J1404.8+6554 | 211.2065 | 65.9088 | BLLAC | 0.189 | 0.061 | 5 | 6,7,8,12b,13 |
| J1406.1−2508 | 211.5400 | −25.1359 | BLLAC | 0.640 | 0.662 | 2 | 3,6 |
| J1406.4−1654 | 211.6592 | −16.8314 | UNCL | 0.420 | 0.187 | 3 | 3,4,6 |
| J1406.6−3934 | 211.6254 | −39.5858 | BLLAC | - | - | - | |
| J1406.9+1643 | 211.7467 | 16.7017 | BLLAC | 0.339 | 0.286 | 2 | 3,13 |
| J1407.5−2706 | 211.8149 | −27.1582 | BLLAC | 0.047 | 0.026 | 3 | 5,6,11 |
| J1407.6−4301 | 211.9155 | −43.0422 | BLLAC | - | - | - | |
| J1408.9−0751 | 212.2353 | −7.8741 | FSRQ | 0.667 | 0.341 | 2 | 3,13 |
| J1410.1+0202 | 212.5194 | 2.0519 | BLLAC | 1.240 | 1.040 | 2 | 3,13 |
| J1410.3+1438 | 212.6169 | 14.6445 | BLLAC | 0.105 | 0.019 | 7 | 5,6,7,8,10,11,13 |
| J1410.3+6058 | 212.6285 | 61.0036 | BLLAC | 0.239 | 0.053 | 5 | 6,7,8,12b,13 |
| J1410.4+2820 | 212.6232 | 28.3488 | BLLAC | 0.482 | 0.430 | 3 | 3,6,13 |
| J1410.5+6215 | 212.6476 | 62.2798 | UNCL | 0.582 | 0.364 | 5 | 7,8,11,12b,13 |
| J1411.5−0723 | 212.8889 | −7.3815 | BLLAC | 0.283 | 0.046 | 5 | 4,6,11,12b,13 |
| J1411.8+5249 | 212.9560 | 52.8167 | MIS | 0.058 | 0.014 | 8 | 5,6,7,8,10,11,12b,13 |
| J1412.0+3836 | 213.0342 | 38.5892 | BLLAC | 0.949 | 0.579 | 4 | 1,3,4,13 |
| J1412.1+7427 | 212.8944 | 74.4083 | BLLAC | 0.542 | 0.631 | 2 | 3,13 |
| J1412.9+5018 | 213.2595 | 50.3242 | FSRQ | 1.033 | 0.131 | 3 | 1,3,13 |
| J1415.5+4830 | 213.9033 | 48.5085 | BLLAC | 0.468 | 0.304 | 3 | 1,3,13 |
| J1415.9−1002 | 213.8368 | −9.9329 | FSRQ | 0.826 | - | 1 | 3 |
| J1416.1+1320 | 213.9951 | 13.3399 | AMB | 0.334 | 0.030 | 6 | 6,7,8,11,12b,13 |
| J1416.1−2417 | 214.0507 | −24.3038 | BLLAC | 0.095 | 0.013 | 3 | 5,6,11 |
| J1417.9+2543 | 214.4861 | 25.7240 | BLLAC | 0.128 | 0.058 | 6 | 5,6,7,8,11,13 |
| J1417.9+4613 | 214.2840 | 46.1182 | FSRQ | 0.855 | 1.044 | 2 | 3,13 |
| J1418.4+3543 | 214.6191 | 35.7137 | FSRQ | 0.485 | 0.268 | 5 | 1,3,4,6,13 |
| J1418.4−0233 | 214.6097 | −2.5595 | BLLAC | 0.075 | - | 1 | 13 |
| J1418.7−3504 | 214.7455 | −35.1618 | FSRQ | 0.244 | - | 1 | 6 |
| J1418.9+7731 | 214.7515 | 77.5415 | BLLAC | 1.216 | 1.543 | 2 | 3,13 |
| J1419.3+0444 | 214.8645 | 4.7538 | AMB | 0.809 | 0.908 | 4 | 1,3,8,13 |
| J1419.4−0838 | 214.8440 | −8.6423 | FSRQ | 0.713 | 0.371 | 3 | 3,6,13 |
| J1419.5+3821 | 214.9442 | 38.3635 | FSRQ | 1.082 | 0.293 | 3 | 1,3,13 |
| J1419.8+5423 | 214.9442 | 54.3874 | BLLAC | 0.253 | 0.225 | 3 | 3,6,13 |
| J1420.3+0612 | 215.0570 | 6.2413 | BLLAC | 0.974 | 1.155 | 2 | 1,13 |
| J1420.9−7920 | 215.3499 | −79.3407 | UNCL | - | - | - | |
| J1421.1+3859 | 215.2751 | 38.9230 | FSRQ | 0.347 | 0.154 | 4 | 1,3,6,13 |
| J1421.1−1120 | 215.2506 | −11.3057 | UNCL | 1.168 | - | 1 | 3 |
| J1421.1−4614 | 215.1977 | −46.2415 | UNCL | - | - | - | |
| J1421.6−4819 | 215.4110 | −48.3397 | FSRQ | 0.538 | - | 1 | 6 |
| J1422.3+3223 | 215.6266 | 32.3862 | CLAGN | 0.515 | 0.263 | 4 | 1,3,6,13 |
| J1422.6+5801 | 215.6620 | 58.0321 | BLLAC | 0.445 | 0.001 | 2 | 1,13 |
| J1423.1+3738 | 215.7692 | 37.6252 | BLLAC | 0.454 | 0.306 | 3 | 1,3,13 |
| J1423.5+4524 | 215.8697 | 45.3955 | BLLAC | 0.749 | 0.137 | 5 | 7,8,11,12b,13 |
| J1423.5−7829 | 215.9315 | −78.4930 | FSRQ | 0.717 | - | 1 | 6 |
| J1424.1+2917 | 216.0347 | 29.3001 | BLLAC | 0.368 | 0.148 | 6 | 1,3,6,11,12b,13 |
| J1424.1−1750 | 216.0515 | −17.8357 | BLLAC | 0.056 | 0.002 | 3 | 5,6,11 |
| J1424.2+0433 | 216.0396 | 4.5811 | BLLAC | 0.452 | 0.466 | 2 | 3,13 |
| J1424.6+1447 | 216.1512 | 14.8196 | BLLAC | 0.557 | 0.481 | 3 | 1,3,13 |
| J1425.0+3615 | 216.2313 | 36.2600 | BLLAC | 0.470 | 0.390 | 2 | 3,13 |
| J1425.4−0119 | 216.3590 | −1.3072 | BLLAC | 0.511 | 0.127 | 4 | 1,3,4,13 |
| J1426.1+3403 | 216.5322 | 34.0740 | BLLAC | 0.489 | 0.433 | 2 | 3,13 |
| J1426.4+3625 | 216.6545 | 36.4193 | FSRQ | 0.867 | 0.345 | 3 | 1,3,13 |
| J1427.0+2348 | 216.7516 | 23.8000 | BLLAC | 0.026 | - | 1 | 13 |
| J1427.4−1823 | 216.8580 | −18.3845 | UNCL | 0.678 | 0.393 | 3 | 3,4,6 |
| J1427.6−3305 | 216.9223 | −33.0921 | BLLAC | 0.404 | - | 1 | 6 |
| J1427.7−3215 | 216.9592 | −32.2547 | UNCL | 0.208 | - | 1 | 6 |
| J1427.9−4206 | 216.9846 | −42.1054 | FSRQ | - | - | - | |
| J1428.1+1629 | 217.0474 | 16.4811 | FSRQ | 0.259 | 0.142 | 6 | 1,6,7,8,11,13 |
| J1428.3+5635 | 217.1031 | 56.6031 | FSRQ | 1.258 | 0.855 | 4 | 1,3,6,13 |
| J1428.5+4240 | 217.1359 | 42.6725 | BLLAC | 0.074 | 0.025 | 5 | 5,6,7,8,13 |
| J1428.7−1017 | 217.1873 | −10.2841 | UNCL | 1.233 | 0.357 | 2 | 3,4 |
| J1428.8+7429 | 217.1247 | 74.5006 | UNCL | 0.245 | 0.036 | 4 | 4,6,12b,13 |
| J1428.9+5406 | 217.3412 | 54.1031 | FSRQ | 1.748 | 0.801 | 3 | 1,3,13 |
| J1429.8−3058 | 217.4160 | −31.0036 | UNCL | 0.265 | 0.087 | 2 | 4,11 |
| J1431.1−3120 | 217.7884 | −31.3441 | UNCL | 0.150 | 0.182 | 2 | 6,11 |
| J1432.8+7648 | 218.0484 | 76.7322 | UNCL | 0.840 | 0.584 | 4 | 3,4,6,13 |
| J1433.0−1801 | 218.2404 | −18.0265 | FSRQ | 2.326 | - | 1 | 3 |
| J1433.7−7304 | 218.4282 | −73.0772 | BLLAC | 0.147 | - | 1 | 6 |
| J1434.2+4204 | 218.5237 | 42.0544 | FSRQ | 0.730 | 0.242 | 3 | 1,3,13 |
| J1434.7+1950 | 218.6658 | 19.8669 | FSRQ | 0.877 | 0.475 | 3 | 1,3,13 |
| J1434.8+6640 | 218.6727 | 66.6740 | BLLAC | 0.574 | 0.231 | 3 | 3,4,13 |
| J1435.5+2021 | 218.8414 | 20.3550 | MIS | 0.442 | 0.375 | 5 | 1,3,5,6,13 |
| J1435.9−8348 | 218.3685 | −83.6858 | UNCL | - | - | - | |
| J1436.9+2321 | 219.1708 | 23.3509 | FSRQ | 0.709 | 0.206 | 3 | 1,3,13 |
| J1436.9+5638 | 219.2405 | 56.6569 | BLLAC | 0.274 | 0.230 | 2 | 1,13 |
| J1438.0−3128 | 219.5449 | −31.3746 | FSRQ | - | - | - | |
| J1438.5−4207 | 219.6531 | −42.1186 | UNCL | - | - | - | |
| J1438.6+1205 | 219.6065 | 12.0719 | BLLAC | 0.413 | 0.074 | 3 | 1,6,13 |
| J1438.9+3710 | 219.7234 | 37.1765 | FSRQ | 1.613 | 0.527 | 4 | 1,3,4,13 |
| J1439.3+3932 | 219.8228 | 39.5452 | BLLAC | 0.125 | 0.032 | 2 | 6,13 |
| J1439.5−2525 | 219.8944 | −25.4164 | BLLAC | 0.141 | 0.019 | 3 | 5,6,11 |
| J1439.7+4958 | 219.9457 | 49.9682 | BLLAC | 0.614 | 0.602 | 2 | 3,13 |
| J1439.9−3953 | 219.9619 | −39.9218 | BLLAC | - | - | - | |
| J1440.0−1530 | 219.9870 | −15.5307 | BLLAC | 0.702 | 0.287 | 2 | 3,6 |
| J1440.0−2343 | 219.9977 | −23.6947 | BLLAC | 0.239 | 0.081 | 2 | 4,6 |
| J1440.6−3846 | 220.1576 | −38.7820 | BLLAC | 0.141 | - | 1 | 6 |
| J1440.9+0609 | 220.2206 | 6.1712 | BLLAC | 0.171 | - | 1 | 13 |
| J1441.6−1522 | 220.4392 | −15.3934 | FSRQ | 0.758 | 0.160 | 2 | 3,6 |
| J1441.7+1836 | 220.4313 | 18.6196 | BLLAC | 0.624 | 0.282 | 4 | 1,3,6,13 |
| J1442.0+4348 | 220.5298 | 43.8102 | BLLAC | 0.550 | 0.262 | 4 | 1,3,12c,13 |
| J1442.2+0622 | 220.5510 | 6.4239 | FSRQ | 0.525 | 0.244 | 5 | 3,7,8,12b,13 |
| J1442.6−4623 | 220.6517 | −46.3838 | BLLAC | 0.085 | 0.016 | 2 | 5,6 |
| J1442.7+1200 | 220.7012 | 12.0112 | BLLAC | 0.105 | 0.039 | 6 | 5,6,7,8,11,13 |
| J1443.1+4728 | 220.8273 | 47.4324 | NLS1 | 0.429 | 0.257 | 3 | 1,3,13 |
| J1443.1+5201 | 220.7615 | 52.0270 | MIS | 0.122 | 0.017 | 8 | 5,6,7,8,10,11,12b,13 |
| J1443.6+2515 | 220.8933 | 25.2662 | BLLAC | 0.483 | 0.044 | 3 | 1,12b,13 |
| J1443.9+2501 | 220.9871 | 25.0290 | FSRQ | 0.539 | 0.370 | 3 | 1,3,13 |
| J1443.9−3908 | 220.9883 | −39.1445 | BLLAC | 0.059 | - | 1 | 6 |
| J1445.0−0326 | 221.2760 | −3.4369 | BLLAC | 0.119 | 0.029 | 2 | 6,13 |
| J1445.9−1626 | 221.4724 | −16.4838 | BLLAC | 0.989 | - | 1 | 3 |
| J1446.0−3039 | 221.4834 | −30.6182 | UNCL | - | - | - | |
| J1446.3+3111 | 221.6515 | 31.1795 | BLLAC | 0.079 | - | 1 | 13 |
| J1446.7+1719 | 221.6473 | 17.3521 | FSRQ | 0.756 | 0.270 | 4 | 1,3,6,13 |
| J1446.8−1830 | 221.6868 | −18.4903 | UNCL | 0.814 | 0.700 | 2 | 3,6 |
| J1447.0−2657 | 221.7369 | −26.9495 | BLLAC | 0.174 | - | 1 | 6 |
| J1448.0+3608 | 222.0024 | 36.1420 | BLLAC | 0.449 | 0.464 | 2 | 3,13 |
| J1449.5+2746 | 222.3664 | 27.7806 | MIS | 0.039 | 0.023 | 7 | 5,6,7,8,10,12b,13 |
| J1449.6−2137 | 222.4166 | −21.6569 | FSRQ | 0.897 | - | 1 | 3 |
| J1449.7−0910 | 222.4245 | −9.1669 | UNCL | 0.159 | 0.034 | 4 | 4,5,6,11 |
| J1450.4+0910 | 222.6299 | 9.1744 | FSRQ | 1.211 | 0.748 | 4 | 1,3,6,13 |
| J1450.8+5201 | 222.7499 | 52.0199 | BLLAC | 0.369 | 0.155 | 3 | 1,3,13 |
| J1451.4+6355 | 222.8655 | 63.9054 | BLLAC | 0.261 | 0.249 | 2 | 6,13 |
| J1451.5+1415 | 222.8624 | 14.2741 | MIS | 0.459 | 0.060 | 6 | 6,7,8,11,12b,13 |
| J1451.8−3851 | 223.0219 | −38.8555 | UNCL | 0.204 | - | 1 | 6 |
| J1453.0−1318 | 223.2423 | −13.3230 | UNCL | - | - | - | |
| J1453.5+3505 | 223.3273 | 35.0943 | BLLAC | 0.432 | 0.161 | 3 | 1,3,13 |
| J1454.0+4927 | 223.5536 | 49.4445 | FSRQ | 1.195 | 0.788 | 4 | 1,3,6,13 |
| J1454.1+1622 | 223.5869 | 16.4068 | FSRQ | 1.084 | 0.525 | 3 | 1,3,13 |
| J1454.1+2647 | 223.4733 | 26.8093 | BLLAC | 0.757 | 0.157 | 3 | 1,3,13 |
| J1454.4+5124 | 223.6130 | 51.4094 | BLLAC | 0.566 | 0.682 | 2 | 3,13 |
| J1454.4−3744 | 223.6142 | −37.7925 | FSRQ | - | - | - | |
| J1455.0+0247 | 223.7810 | 2.8445 | BLLAC | 0.522 | 0.232 | 4 | 1,3,6,13 |
| J1455.4−3654 | 223.7901 | −36.9187 | MIS | 0.071 | 0.025 | 2 | 5,6 |
| J1455.8−7601 | 223.9320 | −76.0145 | BLLAC | - | - | - | |
| J1456.0+5051 | 224.0338 | 50.8101 | BLLAC | 1.131 | 0.002 | 2 | 12b,13 |
| J1457.3−4246 | 224.3042 | −42.8102 | UNCL | 0.358 | - | 1 | 6 |
| J1457.4−3539 | 224.3613 | −35.6528 | FSRQ | - | - | - | |
| J1457.8−4642 | 224.4243 | −46.7028 | BLLAC | 0.082 | 0.022 | 2 | 5,6 |
| J1458.6+3722 | 224.6866 | 37.3393 | BLLAC | 0.545 | 0.363 | 3 | 1,3,13 |
| J1459.0+6129 | 224.7196 | 61.4705 | UNCL | 0.672 | 0.179 | 5 | 7,8,11,12b,13 |
| J1459.0+7140 | 224.7816 | 71.6722 | MIS | 0.555 | 0.480 | 2 | 3,13 |
| J1459.5+1527 | 224.8423 | 15.4485 | BLLAC | 0.460 | 0.147 | 4 | 1,3,6,13 |
| J1500.7+4752 | 225.2027 | 47.8543 | BLLAC | 0.611 | 0.161 | 3 | 1,3,13 |
| J1500.9+5528 | 225.2761 | 55.4641 | BLLAC | 0.503 | 0.038 | 3 | 1,3,13 |
| J1501.0+2238 | 225.2576 | 22.6351 | BLLAC | 0.073 | 0.070 | 2 | 6,13 |
| J1502.5+5552 | 225.6211 | 55.8680 | UNCL | - | - | - | |
| J1503.3+1651 | 225.8194 | 16.8546 | UNCL | 0.674 | 0.555 | 3 | 3,4,13 |
| J1503.5+4759 | 225.8533 | 47.9750 | MIS | 0.337 | 0.269 | 3 | 3,6,13 |
| J1503.7−1540 | 225.9194 | −15.6873 | BLLAC | - | - | - | |
| J1503.9−4247 | 226.0266 | −42.8058 | UNCL | - | - | - | |
| J1504.4+1029 | 226.1041 | 10.4942 | FSRQ | 0.383 | 0.282 | 3 | 1,3,13 |
| J1505.0+0326 | 226.2770 | 3.4419 | NLS1 | 0.359 | 0.116 | 5 | 1,3,6,12b,13 |
| J1505.0−3433 | 226.2599 | −34.5491 | BLLAC | 0.359 | - | 1 | 6 |
| J1505.5−8241 | 226.3561 | −82.7086 | UNCL | 0.329 | 0.095 | 2 | 4,6 |
| J1506.1+3731 | 226.5397 | 37.5142 | FSRQ | 0.595 | 0.048 | 5 | 7,8,11,12b,13 |
| J1506.4+4331 | 226.5735 | 43.5704 | BLLAC | 0.492 | 0.253 | 5 | 1,3,12b,12c,13 |
| J1506.4−0540 | 226.6542 | −5.6681 | BLLAC | 0.375 | 0.150 | 3 | 6,12b,13 |
| J1506.6+0813 | 226.6853 | 8.2335 | BLLAC | 0.592 | 0.679 | 2 | 3,13 |
| J1507.2+1721 | 226.8184 | 17.3508 | BLLAC | 0.436 | 0.390 | 2 | 3,13 |
| J1507.3−3710 | 226.8367 | −37.1508 | UNCL | 0.206 | - | 1 | 6 |
| J1508.4+7717 | 227.0452 | 77.3046 | UNCL | 0.248 | 0.127 | 5 | 3,4,6,12b,13 |
| J1508.8+2708 | 227.1776 | 27.1521 | BLLAC | 0.171 | 0.060 | 7 | 5,6,7,8,11,12b,13 |
| J1509.6−4334 | 227.3989 | −43.6755 | FSRQ | 0.216 | - | 1 | 6 |
| J1509.7+5556 | 227.4498 | 55.9381 | BLLAC | 0.578 | 0.643 | 2 | 3,13 |
| J1509.8−2906 | 227.4377 | −29.0836 | UNCL | - | - | - | |
| J1510.1+5702 | 227.5122 | 57.0454 | FSRQ | 2.138 | 1.885 | 4 | 1,3,6,13 |
| J1510.8+7959 | 227.6364 | 80.0015 | UNCL | 0.868 | 0.295 | 3 | 3,4,13 |
| J1510.8−0542 | 227.7233 | −5.7187 | FSRQ | 0.501 | 0.610 | 2 | 3,13 |
| J1511.8−0513 | 227.9523 | −5.2297 | BLLAC | 0.907 | 1.074 | 2 | 3,13 |
| J1512.1−2255 | 228.0531 | −22.9190 | BLLAC | 1.581 | - | 1 | 3 |
| J1512.2+0202 | 228.0656 | 2.0547 | MIS | 0.244 | 0.131 | 5 | 3,6,7,8,13 |
| J1512.2+4704 | 228.0594 | 47.0592 | BLLAC | 0.532 | 0.231 | 6 | 3,6,7,8,12b,13 |
| J1512.8−0906 | 228.2106 | −9.1000 | FSRQ | 0.690 | - | 1 | 3 |
| J1513.2−7131 | 228.2185 | −71.5315 | UNCL | - | - | - | |
| J1513.4−0753 | 228.3508 | −7.9143 | BLLAC | 0.149 | - | 1 | 6 |
| J1513.4−3231 | 228.4124 | −32.5832 | FSRQ | - | - | - | |
| J1513.4−3721 | 228.3278 | −37.3365 | UNCL | - | - | - | |
| J1514.4−7719 | 228.6833 | −77.3817 | BLLAC | - | - | - | |
| J1514.6−2044 | 228.6397 | −20.7406 | UNCL | 0.349 | 0.186 | 3 | 3,4,6 |
| J1514.7−3617 | 228.6703 | −36.2847 | UNCL | - | - | - | |
| J1514.8−0949 | 228.7073 | −9.8107 | BLLAC | 1.119 | 0.025 | 2 | 3,4 |
| J1516.5+0015 | 229.1676 | 0.2505 | MIS | 0.046 | 0.017 | 8 | 5,6,7,8,10,11,12b,13 |
| J1516.8+2918 | 229.1733 | 29.3026 | BLLAC | 0.115 | 0.022 | 8 | 5,6,7,8,10,11,12b,13 |
| J1516.8+3651 | 229.2052 | 36.8397 | BLLAC | 0.814 | 0.369 | 3 | 1,3,13 |
| J1516.9+1934 | 229.2367 | 19.5369 | BLLAC | 0.503 | 0.308 | 4 | 1,3,6,13 |
| J1517.0+2639 | 229.2608 | 26.6497 | UNCL | 0.549 | 0.113 | 5 | 1,3,4,6,13 |
| J1517.3+6630 | 229.2698 | 66.4582 | UNCL | 0.820 | 0.362 | 2 | 3,13 |
| J1517.7+6525 | 229.4483 | 65.4231 | BLLAC | 0.738 | 0.830 | 2 | 3,13 |
| J1517.7−2422 | 229.4242 | −24.3721 | BLLAC | 0.081 | 0.087 | 3 | 3,5,6 |
| J1518.0−2731 | 229.5150 | −27.5253 | BLLAC | 0.070 | 0.021 | 2 | 5,6 |
| J1518.4+0750 | 229.6111 | 7.8729 | BLLAC | 0.642 | 0.475 | 3 | 1,3,13 |
| J1518.6+0614 | 229.6905 | 6.2323 | MIS | 0.057 | 0.010 | 8 | 5,6,7,8,10,11,12b,13 |
| J1518.6+4044 | 229.6621 | 40.7501 | AMB | 0.059 | 0.007 | 8 | 5,6,7,8,10,11,12b,13 |
| J1520.0−0905 | 229.9962 | −9.0739 | UNCL | 0.902 | - | 1 | 3 |
| J1520.4+5546 | 230.1457 | 55.7158 | BLLAC | 0.480 | 0.264 | 3 | 1,3,13 |
| J1520.5+4209 | 230.1655 | 42.1865 | AMB | 0.325 | 0.272 | 2 | 12c,13 |
| J1520.8−0348 | 230.2038 | −3.8144 | BLLAC | 1.001 | - | 1 | 3 |
| J1521.1+0421 | 230.3439 | 4.3417 | MIS | 0.053 | 0.022 | 6 | 5,6,10,11,12b,13 |
| J1521.8+4338 | 230.4567 | 43.6109 | FSRQ | 1.558 | 0.733 | 3 | 1,3,13 |
| J1522.1+3144 | 230.5416 | 31.7373 | FSRQ | 0.793 | 0.167 | 3 | 1,3,13 |
| J1522.6−2730 | 230.6570 | −27.5030 | BLLAC | 1.056 | - | 1 | 3 |
| J1523.2−3941 | 230.8886 | −39.6115 | UNCL | 0.799 | 0.801 | 2 | 4,6 |
| J1526.1−0831 | 231.5133 | −8.5296 | BLLAC | 0.587 | 0.250 | 2 | 3,4 |
| J1526.7−1529 | 231.6945 | −15.5074 | BLLAC | 0.214 | 0.054 | 4 | 3,4,5,6 |
| J1527.3+3117 | 231.8281 | 31.2568 | FSRQ | 1.061 | 0.324 | 3 | 1,3,13 |
| J1528.2−2905 | 232.0606 | −28.9810 | UNCL | 0.834 | 0.445 | 2 | 3,4 |
| J1529.2+3812 | 232.3065 | 38.2049 | BLLAC | 0.831 | 0.958 | 4 | 1,3,4,13 |
| J1529.7+6733 | 232.4299 | 67.5298 | UNCL | 1.050 | - | 1 | 13 |
| J1530.5−3026 | 232.6714 | −30.4329 | UNCL | - | - | - | |
| J1530.9+5736 | 232.7425 | 57.6070 | BLLAC | 0.724 | 0.294 | 4 | 1,3,4,13 |
| J1531.7+4710 | 232.9158 | 47.1181 | BLLAC | 1.038 | 0.613 | 4 | 1,3,4,13 |
| J1532.0+3016 | 233.0093 | 30.2747 | BLLAC | 0.057 | 0.009 | 8 | 5,6,7,8,10,11,12b,13 |
| J1532.7−1319 | 233.1891 | −13.3195 | UNCL | 0.707 | 0.094 | 3 | 7,8,11 |
| J1533.2+1855 | 233.2969 | 18.9081 | BLLAC | 0.174 | 0.076 | 6 | 6,7,8,11,12b,13 |
| J1533.2+3416 | 233.3511 | 34.2779 | BLLAC | 0.981 | 1.154 | 2 | 3,13 |
| J1534.8+0131 | 233.7186 | 1.5178 | FSRQ | 0.981 | 0.396 | 3 | 1,3,13 |
| J1534.8+3716 | 233.6967 | 37.2652 | BLLAC | 0.119 | 0.041 | 6 | 5,6,7,8,11,13 |
| J1535.0+5320 | 233.7533 | 53.3436 | BLLAC | 1.010 | 1.280 | 2 | 1,13 |
| J1535.3−3135 | 233.8737 | −31.5629 | UNCL | 0.253 | 0.063 | 2 | 4,6 |
| J1535.4+3919 | 233.8712 | 39.3794 | BLLAC | 0.220 | 0.067 | 6 | 3,6,7,8,12b,13 |
| J1536.8−3155 | 234.2271 | −31.8542 | BLLAC | - | - | - | |
| J1537.7−7957 | 234.4199 | −79.9680 | UNCL | - | - | - | |
| J1537.9−1344 | 234.4877 | −13.7220 | UNCL | 0.984 | 0.766 | 2 | 1,3 |
| J1539.6+2743 | 234.9131 | 27.7439 | FSRQ | 1.525 | 0.876 | 2 | 1,13 |
| J1539.7−1127 | 234.9217 | −11.4765 | BLLAC | 0.838 | 0.850 | 2 | 3,4 |
| J1539.9+4220 | 234.8570 | 42.2912 | BLLAC | 0.808 | 0.485 | 2 | 3,13 |
| J1540.1+8155 | 235.0662 | 81.9183 | BLLAC | 0.227 | 0.241 | 4 | 3,5,6,13 |
| J1540.4+6606 | 235.0001 | 66.0976 | UNCL | 0.693 | 0.289 | 4 | 3,4,12b,13 |
| J1540.7+1449 | 235.2062 | 14.7961 | BLLAC | 0.370 | 0.305 | 2 | 3,13 |
| J1541.7+1413 | 235.4587 | 14.2438 | BLLAC | 0.159 | 0.043 | 4 | 6,11,12b,13 |
| J1541.9−2915 | 235.5129 | −29.2526 | BLLAC | 1.403 | - | 1 | 3 |
| J1542.3+1801 | 235.5815 | 17.9355 | MIS | 1.120 | 0.688 | 3 | 1,3,13 |
| J1543.0+6130 | 235.7373 | 61.4987 | BLLAC | 0.528 | 0.652 | 2 | 3,13 |
| J1543.6+0452 | 235.8914 | 4.8720 | BLLAC | 0.024 | 0.010 | 5 | 5,6,11,12b,13 |
| J1544.3−0649 | 236.0819 | −6.8209 | BLLAC | 0.138 | 0.044 | 3 | 4,5,6 |
| J1545.8−2336 | 236.4441 | −23.6580 | BLLAC | 0.106 | 0.012 | 3 | 5,6,11 |
| J1546.0+0819 | 236.5177 | 8.3204 | BLLAC | 1.056 | 1.248 | 2 | 3,13 |
| J1546.1−1003 | 236.5478 | −10.0573 | UNCL | 1.336 | - | 1 | 3 |
| J1546.5+1816 | 236.5988 | 18.2876 | BLLAC | 0.538 | 0.421 | 3 | 1,3,13 |
| J1547.3−2802 | 236.8006 | −28.0393 | UNCL | 0.876 | - | 1 | 3 |
| J1548.3+1456 | 237.1016 | 14.9508 | BLLAC | 0.251 | 0.021 | 7 | 3,6,7,8,11,12b,13 |
| J1548.3+6615 | 237.1305 | 66.2758 | UNCL | 0.461 | 0.131 | 4 | 3,4,6,13 |
| J1548.8−2250 | 237.2073 | −22.8507 | BLLAC | 0.097 | 0.000 | 2 | 5,6 |
| J1549.0+7846 | 237.1561 | 78.7574 | BLLAC | 0.588 | 0.133 | 3 | 3,4,13 |
| J1549.3+4234 | 237.3278 | 42.5835 | BLLAC | 0.799 | 0.527 | 4 | 1,3,4,13 |
| J1549.3+6310 | 237.4888 | 63.1687 | UNCL | 1.254 | 0.798 | 3 | 3,4,13 |
| J1549.4+7409 | 237.3638 | 74.1589 | UNCL | 0.342 | 0.201 | 4 | 3,4,6,13 |
| J1549.5+0236 | 237.3727 | 2.6170 | FSRQ | 0.486 | 0.508 | 2 | 3,13 |
| J1549.6+1710 | 237.3720 | 17.1411 | BLLAC | 0.449 | 0.308 | 4 | 1,3,6,13 |
| J1549.8−0659 | 237.4668 | −6.9855 | BLLAC | 0.557 | 0.390 | 3 | 3,4,6 |
| J1549.8−3044 | 237.4429 | −30.7503 | BLLAC | - | - | - | |
| J1550.7+0528 | 237.6470 | 5.4529 | FSRQ | 0.624 | 0.363 | 3 | 1,3,13 |
| J1550.7+7006 | 237.4852 | 70.2156 | UNCL | 0.937 | 0.347 | 4 | 3,4,6,13 |
| J1550.8−0822 | 237.7220 | −8.3797 | UNCL | 0.284 | 0.021 | 2 | 3,4 |
| J1550.8−1750 | 237.8108 | −17.9173 | UNCL | 1.306 | 0.031 | 2 | 1,3 |
| J1552.0+0850 | 238.0136 | 8.8465 | BLLAC | 0.608 | 0.643 | 2 | 3,13 |
| J1553.3+0600 | 238.3794 | 6.0288 | BLLAC | 0.485 | 0.129 | 5 | 6,7,8,12b,13 |
| J1553.5−3118 | 238.3898 | −31.3087 | BLLAC | 0.084 | - | 1 | 6 |
| J1553.6+1257 | 238.3862 | 12.9477 | FSRQ | 0.809 | 1.044 | 2 | 3,13 |
| J1553.6−2422 | 238.3818 | −24.3683 | SEY | 1.282 | - | 1 | 3 |
| J1554.4−1215 | 238.6358 | −12.2237 | UNCL | 0.625 | 0.474 | 3 | 3,4,6 |
| J1554.9+2143 | 238.7524 | 21.6999 | BLLAC | 0.541 | 0.538 | 2 | 3,13 |
| J1555.7+1111 | 238.9294 | 11.1901 | BLLAC | 0.028 | - | 1 | 13 |
| J1557.5−7040 | 239.4007 | −70.6745 | UNCL | - | - | - | |
| J1557.9−0001 | 239.4643 | −0.0307 | FSRQ | 0.670 | 0.207 | 3 | 1,3,13 |
| J1557.9−1404 | 239.5914 | −14.1664 | SEY | 0.056 | 0.032 | 3 | 5,6,11 |
| J1558.8+5625 | 239.7012 | 56.4206 | BLLAC | 0.397 | 0.290 | 3 | 3,4,13 |
| J1559.1+6736 | 239.7336 | 67.6133 | UNCL | 0.581 | 0.463 | 4 | 3,4,6,13 |
| J1559.8−2525 | 240.0224 | −25.4111 | BLLAC | 0.353 | 0.144 | 3 | 3,4,6 |
| J1559.9+2319 | 239.9675 | 23.2824 | BLLAC | 0.673 | 0.710 | 2 | 3,13 |
| J1600.0+8510 | 240.1321 | 85.1637 | UNCL | 0.986 | - | 1 | 3 |
| J1602.0−0641 | 240.4441 | −6.7156 | UNCL | 1.097 | 1.064 | 2 | 3,4 |
| J1602.1+3324 | 240.5303 | 33.4481 | MIS | 1.044 | 0.065 | 3 | 4,12b,13 |
| J1602.2+3051 | 240.5753 | 30.8526 | BLLAC | 0.861 | 0.969 | 2 | 3,13 |
| J1602.9−1928 | 240.7023 | −19.4965 | UNCL | 1.111 | - | 1 | 3 |
| J1603.5−7112 | 241.3161 | −71.2165 | UNCL | - | - | - | |
| J1603.8+1104 | 240.9247 | 11.0969 | BLLAC | 0.475 | 0.473 | 3 | 3,6,13 |
| J1603.8+5009 | 240.9146 | 50.1654 | BLLAC | 0.471 | 0.029 | 2 | 1,13 |
| J1604.6+5714 | 241.1556 | 57.2435 | FSRQ | 0.567 | 0.355 | 3 | 1,3,13 |
| J1604.7+1734 | 241.1525 | 17.5567 | BLLAC | 0.674 | 0.467 | 4 | 1,3,6,13 |
| J1604.9−3414 | 241.2305 | −34.2341 | UNCL | - | - | - | |
| J1605.1−1140 | 241.3230 | −11.6575 | BLLAC | 1.052 | 0.197 | 2 | 3,4 |
| J1605.5+5423 | 241.3292 | 54.3497 | BLLAC | 0.212 | 0.043 | 5 | 6,7,8,12b,13 |
| J1605.8+7208 | 241.3987 | 72.1479 | AMB | 0.407 | 0.097 | 3 | 4,6,13 |
| J1606.2+1346 | 241.5766 | 13.7591 | BLLAC | 0.178 | 0.072 | 6 | 6,7,8,11,12b,13 |
| J1606.3+5629 | 241.5858 | 56.5053 | SEY | 0.265 | 0.015 | 3 | 6,7,8 |
| J1606.5+2717 | 241.7429 | 27.2849 | FSRQ | 0.695 | 0.463 | 3 | 1,3,13 |
| J1606.6+1324 | 241.7277 | 13.3261 | UNCL | - | - | - | |
| J1607.0+1550 | 241.7768 | 15.8596 | BLLAC | 0.439 | 0.145 | 5 | 1,3,6,12b,13 |
| J1608.0−2038 | 241.9872 | −20.6618 | UNCL | - | - | - | |
| J1608.3+4012 | 242.0923 | 40.2050 | FSRQ | 0.621 | 0.204 | 5 | 1,3,6,12b,13 |
| J1608.7+1029 | 242.1925 | 10.4855 | FSRQ | 0.697 | 0.421 | 3 | 1,3,13 |
| J1610.6+2414 | 242.6751 | 24.2469 | FSRQ | 0.833 | 0.407 | 4 | 1,3,6,13 |
| J1610.7−6648 | 242.6936 | −66.8170 | BLLAC | 0.100 | - | 1 | 4 |
| J1612.4−0554 | 243.1198 | −5.9650 | BLLAC | 0.021 | 0.011 | 3 | 5,6,11 |
| J1612.4−3100 | 243.0834 | −30.9941 | BLLAC | 0.900 | - | 1 | 4 |
| J1613.3−1907 | 243.3632 | −19.1434 | UNCL | 0.632 | 0.443 | 2 | 3,4 |
| J1613.6+3411 | 243.4211 | 34.2133 | FSRQ | 0.532 | 0.575 | 3 | 3,6,13 |
| J1614.8−0850 | 243.6833 | −8.8557 | UNCL | 0.344 | 0.209 | 2 | 4,6 |
| J1615.6+2130 | 243.8796 | 21.5031 | FSRQ | 0.638 | 0.185 | 4 | 1,3,6,13 |
| J1615.6+4712 | 243.9217 | 47.1866 | MIS | 0.165 | 0.063 | 6 | 3,5,6,7,8,13 |
| J1616.6+4630 | 244.0157 | 46.5403 | FSRQ | 1.114 | 0.116 | 3 | 1,3,13 |
| J1616.7+3327 | 244.1407 | 33.5121 | BLLAC | 0.572 | 0.255 | 3 | 1,3,13 |
| J1616.7+4107 | 244.2764 | 41.1131 | BLLAC | 0.186 | 0.063 | 7 | 3,6,7,8,11,12b,13 |
| J1617.2−2535 | 244.3357 | −25.6232 | UNCL | 1.813 | - | 1 | 3 |
| J1617.3−1513 | 244.3055 | −15.1830 | UNCL | 0.100 | - | 1 | 4 |
| J1617.9−7718 | 244.4553 | −77.2885 | FSRQ | 0.197 | - | 1 | 6 |
| J1618.0+5139 | 244.3728 | 51.6723 | FSRQ | 1.834 | 0.447 | 3 | 1,3,13 |
| J1618.8+0620 | 244.6275 | 6.3697 | BLLAC | 0.520 | 0.045 | 3 | 1,3,13 |
| J1619.0+7536 | 244.8073 | 75.6315 | UNCL | 0.527 | - | 1 | 13 |
| J1619.0−8346 | 244.9593 | −83.8246 | UNCL | 0.063 | 0.005 | 2 | 5,6 |
| J1619.6+5536 | 244.8335 | 55.6010 | BLLAC | 0.464 | 0.254 | 3 | 1,3,13 |
| J1621.7−1103 | 245.4583 | −11.0325 | UNCL | - | - | - | |
| J1623.4+0858 | 245.8773 | 8.9567 | BLLAC | 0.482 | 0.190 | 4 | 1,3,6,13 |
| J1623.6+5743 | 246.1034 | 57.6879 | CLAGN | 0.556 | 0.144 | 3 | 1,3,13 |
| J1624.6+5651 | 246.1341 | 56.8744 | BLLAC | 0.605 | 0.522 | 2 | 3,13 |
| J1625.7+4134 | 246.4903 | 41.5780 | FSRQ | 1.038 | 0.459 | 4 | 3,7,8,13 |
| J1625.7−2527 | 246.4454 | −25.4606 | FSRQ | 1.311 | - | 1 | 3 |
| J1626.0-2950 | 246.5251 | -29.8575 | FSRQ | 1.121 | - | 1 | 3 |
| J1626.3+3514 | 246.6078 | 35.2282 | BLLAC | 0.402 | 0.120 | 3 | 1,4,13 |
| J1626.6−7639 | 246.6590 | −76.6488 | BLLAC | 0.095 | 0.012 | 2 | 5,6 |
| J1626.8+4337 | 246.4721 | 43.7872 | FSRQ | 0.801 | 0.287 | 3 | 1,3,13 |
| J1627.3+3148 | 246.8041 | 31.8322 | BLLAC | 0.603 | 0.124 | 3 | 1,3,13 |
| J1627.3+4758 | 246.9426 | 48.0569 | FSRQ | 1.094 | 0.887 | 4 | 1,3,6,13 |
| J1627.4−3301 | 246.8546 | −33.0562 | UNCL | - | - | - | |
| J1627.7+0251 | 246.9756 | 2.8526 | UNCL | 0.472 | 0.205 | 3 | 3,4,13 |
| J1628.3−3343 | 247.0829 | −33.7282 | UNCL | - | - | - | |
| J1628.6+7706 | 247.1377 | 77.1139 | BLLAC | 0.410 | 0.240 | 5 | 1,3,4,6,13 |
| J1630.6+8234 | 248.1332 | 82.5379 | MIS | 0.020 | 0.012 | 4 | 5,6,11,13 |
| J1630.7+5221 | 247.6798 | 52.3607 | BLLAC | 0.492 | 0.574 | 2 | 3,13 |
| J1631.2+1046 | 247.8282 | 10.8673 | UNCL | 0.866 | 0.178 | 4 | 1,3,4,13 |
| J1631.2+4926 | 247.8189 | 49.4610 | SEY | 0.407 | 0.164 | 5 | 3,6,7,8,13 |
| J1632.4+5800 | 248.0577 | 58.0146 | UNCL | 0.234 | 0.054 | 4 | 4,6,12b,13 |
| J1632.8−1048 | 248.2088 | −10.8756 | UNCL | 1.259 | 0.134 | 3 | 1,3,4 |
| J1635.2+3808 | 248.8146 | 38.1346 | FSRQ | 1.141 | 1.383 | 2 | 3,13 |
| J1635.6+3500 | 248.7782 | 34.9812 | BLLAC | 0.520 | 0.301 | 3 | 1,3,13 |
| J1635.6+3628 | 248.9468 | 36.4917 | FSRQ | 1.919 | 1.343 | 2 | 1,13 |
| J1636.3+7128 | 248.9672 | 71.4816 | FSRQ | 0.226 | 0.193 | 4 | 3,5,6,13 |
| J1636.5−0454 | 249.1333 | −4.9184 | UNCL | 0.174 | 0.051 | 4 | 6,7,8,11 |
| J1636.7+2627 | 249.2145 | 26.4491 | BLLAC | 0.440 | 0.386 | 2 | 3,13 |
| J1637.1+1316 | 249.3197 | 13.2441 | BLLAC | 0.979 | 0.883 | 3 | 1,3,13 |
| J1637.2+4327 | 249.2896 | 43.4334 | BLLAC | 0.179 | 0.057 | 8 | 3,6,7,8,11,12b,12c,13 |
| J1637.6+4548 | 249.3611 | 45.7970 | BLLAC | 0.147 | 0.037 | 7 | 5,6,7,8,11,12b,13 |
| J1637.7+4717 | 249.4380 | 47.2927 | FSRQ | 0.696 | 0.207 | 3 | 1,3,13 |
| J1637.7+7326 | 249.5069 | 73.4377 | BLLAC | 0.892 | 0.896 | 2 | 3,13 |
| J1638.1+5721 | 249.5561 | 57.3400 | FSRQ | 0.442 | 0.572 | 2 | 3,13 |
| J1639.2+4129 | 249.8159 | 41.4760 | FSRQ | 0.852 | 0.729 | 3 | 1,3,13 |
| J1640.2+0629 | 250.0461 | 6.4742 | BLLAC | 0.437 | 0.314 | 3 | 3,4,13 |
| J1640.3+6850 | 250.0623 | 68.8761 | UNCL | 0.715 | 0.778 | 3 | 3,4,13 |
| J1640.4+3945 | 250.1235 | 39.7795 | FSRQ | 0.945 | 0.257 | 3 | 1,3,13 |
| J1640.9+1143 | 250.2454 | 11.7345 | BLLAC | 0.043 | 0.007 | 7 | 5,6,7,8,11,12b,13 |
| J1641.9−0621 | 250.5091 | −6.3566 | BLLAC | 0.718 | 0.406 | 2 | 1,3 |
| J1642.3−8108 | 250.7389 | −81.1431 | BLLAC | - | - | - | |
| J1642.4+2211 | 250.5846 | 22.1953 | BLLAC | 0.372 | 0.091 | 2 | 1,13 |
| J1642.9+3948 | 250.7450 | 39.8103 | FSRQ | 0.368 | 0.348 | 2 | 3,13 |
| J1643.0+3223 | 250.7544 | 32.3511 | BLLAC | 1.421 | 0.776 | 3 | 1,3,13 |
| J1643.0−7714 | 251.0672 | −77.2636 | MIS | - | - | - | |
| J1643.5−0646 | 250.8705 | −6.7722 | BLLAC | 0.060 | 0.031 | 3 | 5,6,11 |
| J1643.7+3317 | 250.9144 | 33.2800 | BLLAC | 0.492 | 0.115 | 6 | 4,6,7,8,12b,13 |
| J1644.2+4546 | 251.0832 | 45.7790 | BLLAC | 0.166 | 0.046 | 7 | 5,6,7,8,11,12b,13 |
| J1644.9+2620 | 251.1772 | 26.3203 | NLS1 | 0.184 | 0.094 | 5 | 3,6,7,8,13 |
| J1645.6+6329 | 251.4940 | 63.5030 | FSRQ | 0.689 | 0.272 | 3 | 1,3,13 |
| J1646.0−0942 | 251.5049 | −9.6884 | UNCL | 0.187 | - | 1 | 6 |
| J1646.6+7422 | 251.5632 | 74.3197 | UNCL | 0.920 | - | 1 | 13 |
| J1646.7−1330 | 251.7157 | −13.4800 | UNCL | 0.300 | - | 1 | 4 |
| J1647.4−6438 | 251.9073 | −64.6334 | BLLAC | 0.360 | - | 1 | 6 |
| J1647.5+2911 | 251.8620 | 29.1638 | BLLAC | 0.099 | 0.019 | 8 | 5,6,7,8,10,11,12b,13 |
| J1647.5+4950 | 251.8955 | 49.8335 | SEY | 0.089 | 0.081 | 9 | 3,5,6,7,8,10,11,12b,13 |
| J1648.0+2221 | 252.0064 | 22.4092 | BLLAC | 0.762 | 0.107 | 5 | 7,8,11,12b,13 |
| J1648.2+4232 | 252.1313 | 42.5562 | FSRQ | - | - | - | |
| J1649.4+5235 | 252.3541 | 52.5875 | BLLAC | 0.292 | 0.261 | 2 | 3,13 |
| J1649.6+0411 | 252.3653 | 4.2011 | UNCL | 0.712 | 0.337 | 4 | 1,3,4,13 |
| J1650.7+0831 | 252.6565 | 8.4145 | FSRQ | 0.725 | 0.394 | 2 | 3,13 |
| J1650.9+0429 | 252.7229 | 4.5026 | UNCL | - | - | - | |
| J1651.6+7219 | 252.9165 | 72.3069 | BLLAC | 0.114 | 0.115 | 2 | 4,13 |
| J1652.7+4024 | 253.2080 | 40.3862 | BLLAC | 0.669 | 0.610 | 3 | 1,3,13 |
| J1653.8+3945 | 253.4676 | 39.7602 | BLLAC | 0.029 | 0.018 | 4 | 5,6,10,13 |
| J1656.0+2047 | 253.9440 | 20.7563 | UNCL | 1.083 | - | 1 | 13 |
| J1656.9−2010 | 254.2298 | −20.1823 | BLLAC | - | - | - | |
| J1657.0+6010 | 254.2010 | 60.2046 | FSRQ | 0.637 | 0.258 | 3 | 3,12b,13 |
| J1657.7+4808 | 254.4453 | 48.1425 | CLAGN | 0.683 | 0.265 | 4 | 3,7,8,13 |
| J1657.7−6120 | 254.4542 | −61.3605 | UNCL | - | - | - | |
| J1658.4+6150 | 254.5347 | 61.8339 | BLLAC | 0.197 | 0.040 | 5 | 6,7,8,12b,13 |
| J1659.0+2627 | 254.8506 | 26.4936 | FSRQ | 0.525 | 0.347 | 3 | 1,3,13 |
| J1700.0+6830 | 255.0387 | 68.5019 | NLS1 | 0.182 | 0.168 | 2 | 6,13 |
| J1701.0+6613 | 255.2466 | 66.2076 | UNCL | 0.795 | 0.277 | 4 | 1,3,4,13 |
| J1701.3+3956 | 255.3526 | 39.9103 | BLLAC | 0.317 | 0.230 | 3 | 3,6,13 |
| J1702.2+2642 | 255.5401 | 26.7207 | BLLAC | 0.632 | 0.642 | 2 | 3,13 |
| J1702.6+3114 | 255.6606 | 31.2621 | BLLAC | 0.702 | 0.714 | 4 | 1,3,4,13 |
| J1703.6−6213 | 255.9023 | −62.2111 | FSRQ | 0.258 | - | 1 | 6 |
| J1704.1+7647 | 255.9912 | 76.7695 | UNCL | 0.592 | 0.262 | 4 | 1,3,4,13 |
| J1704.2+1234 | 256.0399 | 12.5726 | BLLAC | 0.344 | 0.173 | 4 | 1,3,6,13 |
| J1704.5−0527 | 256.1410 | −5.4780 | BLLAC | 1.260 | 1.281 | 2 | 3,4 |
| J1705.0+7134 | 256.1957 | 71.6382 | BLLAC | 0.462 | 0.310 | 3 | 1,3,13 |
| J1705.5−7423 | 256.4615 | −74.3759 | UNCL | 0.206 | - | 1 | 6 |
| J1706.1+1000 | 256.4841 | 10.0049 | UNCL | 0.346 | 0.037 | 5 | 7,8,11,12b,13 |
| J1706.9+4543 | 256.8241 | 45.6032 | FSRQ | 0.479 | 0.600 | 2 | 3,13 |
| J1707.5+1649 | 256.8815 | 16.8124 | SEY | 0.368 | 0.194 | 4 | 1,3,6,13 |
| J1707.9+0016 | 256.9351 | 0.2970 | UNCL | 0.841 | 0.565 | 4 | 1,3,4,6 |
| J1709.7+4318 | 257.4212 | 43.3124 | FSRQ | 0.456 | 0.218 | 3 | 1,3,13 |
| J1710.1−2030 | 257.5405 | −20.5085 | UNCL | - | - | - | |
| J1712.7+2932 | 258.2033 | 29.5213 | BLLAC | 0.304 | 0.331 | 4 | 3,7,8,13 |
| J1713.7+8844 | 258.9721 | 88.7376 | UNCL | 0.625 | 0.166 | 2 | 3,4 |
| J1714.0−2029 | 258.5227 | −20.4637 | UNCL | - | - | - | |
| J1715.0+2616 | 258.7076 | 26.2384 | UNCL | 0.310 | 0.099 | 8 | 3,4,6,7,8,11,12b,13 |
| J1715.8+2151 | 259.0466 | 21.8705 | FSRQ | 0.354 | 0.071 | 6 | 3,6,7,8,12b,13 |
| J1716.1+6836 | 259.0581 | 68.6108 | FSRQ | 0.431 | 0.339 | 3 | 3,6,13 |
| J1716.6−6707 | 259.0931 | −67.1067 | BLLAC | 0.157 | - | 1 | 6 |
| J1717.3−6045 | 259.2327 | −60.7624 | UNCL | - | - | - | |
| J1717.5−8114 | 259.2978 | −81.2527 | UNCL | 0.059 | 0.008 | 2 | 5,6 |
| J1719.2+1745 | 259.8044 | 17.7518 | BLLAC | 0.397 | 0.382 | 2 | 3,13 |
| J1719.3+1205 | 259.8396 | 12.1228 | UNCL | 0.407 | 0.282 | 3 | 3,4,13 |
| J1720.2+3824 | 260.0431 | 38.4323 | AMB | 0.361 | 0.086 | 6 | 3,6,7,8,12b,13 |
| J1722.6+6104 | 260.6669 | 61.0999 | FSRQ | 1.399 | 0.673 | 4 | 1,3,6,13 |
| J1722.7+1014 | 260.6858 | 10.2266 | FSRQ | 0.450 | 0.145 | 4 | 1,3,6,13 |
| J1723.6−7714 | 260.9619 | −77.2307 | UNCL | - | - | - | |
| J1724.1+3304 | 261.0592 | 33.0511 | SEY | 0.391 | 0.096 | 5 | 3,6,7,8,13 |
| J1724.2+4005 | 261.0226 | 40.0768 | BLLAC | 0.545 | 0.220 | 6 | 3,7,8,11,12b,13 |
| J1724.2−6501 | 260.9210 | −65.0102 | MIS | 0.010 | 0.004 | 2 | 5,6 |
| J1724.9+7654 | 260.9977 | 76.8865 | FSRQ | 0.485 | 0.303 | 3 | 1,3,13 |
| J1725.0+1152 | 261.2681 | 11.8710 | BLLAC | 0.028 | - | 1 | 13 |
| J1725.4+5254 | 261.3347 | 52.9171 | BLLAC | 0.068 | 0.015 | 8 | 5,6,7,8,10,11,12b,13 |
| J1725.5+5851 | 261.3959 | 58.8611 | BLLAC | 0.399 | 0.394 | 2 | 3,13 |
| J1727.2+0644 | 261.8335 | 6.6893 | UNCL | - | - | - | |
| J1727.4+4530 | 261.8652 | 45.5110 | FSRQ | 0.467 | 0.384 | 3 | 1,3,13 |
| J1727.9−0654 | 261.9655 | −6.9690 | UNCL | - | - | - | |
| J1728.0+1216 | 262.0294 | 12.2610 | FSRQ | 0.857 | 0.328 | 2 | 3,13 |
| J1728.3+5013 | 262.0776 | 50.2196 | BLLAC | 0.056 | 0.016 | 5 | 5,6,11,12b,13 |
| J1728.4+0427 | 262.1040 | 4.4514 | FSRQ | 0.224 | 0.007 | 2 | 3,6 |
| J1728.5−7303 | 261.5046 | −73.0000 | UNCL | - | - | - | |
| J1728.6−7448 | 262.1886 | −74.8976 | UNCL | - | - | - | |
| J1730.6+0024 | 262.6458 | 0.4107 | FSRQ | 0.541 | 0.149 | 2 | 3,6 |
| J1730.6+3805 | 262.6866 | 38.0819 | UNCL | 0.166 | 0.020 | 5 | 4,6,11,12b,13 |
| J1730.8+3715 | 262.6960 | 37.2486 | BLLAC | 0.135 | 0.037 | 6 | 3,5,6,7,8,13 |
| J1733.0−1305 | 263.2613 | −13.0804 | FSRQ | 0.999 | - | 1 | 3 |
| J1733.4+5428 | 263.4180 | 54.4435 | BLLAC | 0.401 | 0.026 | 6 | 6,7,8,11,12b,13 |
| J1733.6−6054 | 263.4101 | −60.9283 | UNCL | - | - | - | |
| J1734.0+0805 | 263.5022 | 8.1079 | UNCL | - | - | - | |
| J1734.3+3858 | 263.5857 | 38.9643 | FSRQ | 0.526 | 0.596 | 2 | 3,13 |
| J1735.4−1118 | 263.8632 | −11.2929 | UNCL | 0.705 | 0.541 | 2 | 3,6 |
| J1735.8−5932 | 263.9678 | −59.5453 | UNCL | 0.215 | - | 1 | 6 |
| J1736.0+2033 | 264.0219 | 20.5503 | BLLAC | 0.800 | 0.889 | 2 | 3,13 |
| J1736.6+0628 | 264.1191 | 6.5299 | FSRQ | 1.341 | 0.799 | 2 | 1,3 |
| J1738.0+0236 | 264.3947 | 2.6140 | UNCL | 0.177 | 0.008 | 2 | 6,11 |
| J1738.0+8717 | 264.3420 | 87.2957 | UNCL | - | - | - | |
| J1738.3+3228 | 264.6688 | 32.4025 | SEY | 0.108 | 0.038 | 4 | 3,5,6,13 |
| J1738.8+3822 | 264.6770 | 38.3507 | UNCL | 0.244 | 0.049 | 5 | 4,6,11,12b,13 |
| J1739.5+4955 | 264.8641 | 49.9176 | FSRQ | 0.984 | 0.386 | 2 | 3,13 |
| J1740.0+4737 | 264.9880 | 47.6329 | BLLAC | 0.570 | 0.114 | 3 | 1,3,13 |
| J1740.5+5211 | 265.1541 | 52.1954 | FSRQ | 0.537 | 0.597 | 2 | 3,13 |
| J1740.6+5346 | 265.1522 | 53.7733 | UNCL | 0.755 | 0.396 | 3 | 1,3,13 |
| J1741.1+7226 | 265.3452 | 72.4144 | BLLAC | 0.134 | 0.053 | 6 | 3,5,6,11,12b,13 |
| J1741.9+2555 | 265.4482 | 25.9120 | BLLAC | 0.610 | 0.259 | 4 | 1,3,4,13 |
| J1742.5+5944 | 265.6333 | 59.7519 | BLLAC | 0.438 | 0.316 | 3 | 3,4,13 |
| J1743.9+3747 | 265.9485 | 37.7983 | FSRQ | 1.319 | 0.628 | 2 | 3,13 |
| J1744.0+1935 | 265.9910 | 19.5858 | BLLAC | 0.041 | 0.010 | 5 | 5,6,11,12b,13 |
| J1744.2−0353 | 265.9952 | −3.8346 | FSRQ | 1.241 | - | 1 | 3 |
| J1744.4+1851 | 266.0825 | 18.8717 | BLLAC | 0.605 | 0.493 | 4 | 1,3,4,13 |
| J1744.6−5713 | 266.1479 | −57.2530 | UNCL | - | - | - | |
| J1745.1+4731 | 266.2580 | 47.5462 | UNCL | 0.999 | 0.049 | 2 | 3,13 |
| J1745.4−0753 | 266.3629 | −7.8844 | BLLAC | 0.854 | 0.946 | 2 | 3,6 |
| J1745.6+3950 | 266.4073 | 39.8586 | BLLAC | 0.154 | 0.038 | 3 | 11,12b,13 |
| J1746.8−5235 | 266.7737 | −52.6090 | UNCL | - | - | - | |
| J1747.1−5453 | 266.8518 | −54.8393 | UNCL | - | - | - | |
| J1747.2+4937 | 266.7596 | 49.6336 | BLLAC | 0.477 | 0.113 | 3 | 7,8,12b |
| J1747.6−5308 | 266.8342 | −53.1723 | UNCL | - | - | - | |
| J1747.9+4704 | 266.8610 | 46.9808 | BLLAC | 0.785 | 0.302 | 4 | 1,3,6,13 |
| J1748.0+3403 | 267.0242 | 34.0670 | FSRQ | 0.664 | 0.604 | 2 | 3,13 |
| J1748.1+2702 | 267.0698 | 27.0759 | UNCL | 0.644 | 0.263 | 3 | 3,4,13 |
| J1748.6+7005 | 267.1368 | 70.0974 | BLLAC | 0.676 | 0.869 | 2 | 3,13 |
| J1749.0+4321 | 267.2515 | 43.3642 | BLLAC | 0.316 | 0.193 | 2 | 3,13 |
| J1751.5+0938 | 267.8867 | 9.6502 | CLAGN | 1.079 | - | 1 | 3 |
| J1751.6+2921 | 267.9278 | 29.3473 | UNCL | 0.736 | 0.270 | 4 | 3,4,6,13 |
| J1752.1+4531 | 268.1091 | 45.5165 | UNCL | 0.207 | 0.065 | 6 | 6,7,8,11,12b,13 |
| J1753.6−5014 | 268.4106 | −50.2540 | UNCL | - | - | - | |
| J1753.7+2847 | 268.4270 | 28.8014 | FSRQ | 0.766 | 0.458 | 3 | 3,6,13 |
| J1754.2+3212 | 268.5492 | 32.2064 | BLLAC | 0.659 | 0.796 | 2 | 3,13 |
| J1754.5−6425 | 268.6750 | −64.3961 | BLLAC | - | - | - | |
| J1754.7+3444 | 268.7129 | 34.7131 | UNCL | 0.544 | 0.192 | 4 | 3,4,6,13 |
| J1756.3+5522 | 269.0662 | 55.3717 | BLLAC | 1.486 | 1.911 | 2 | 3,13 |
| J1756.6+1553 | 269.1405 | 15.8955 | FSRQ | 0.581 | 0.202 | 2 | 3,6 |
| J1756.9+1531 | 269.2213 | 15.5891 | BLLAC | 0.564 | 0.174 | 3 | 3,4,13 |
| J1757.0+7032 | 269.3052 | 70.5604 | BLLAC | - | - | - | |
| J1758.2+6532 | 269.3497 | 65.6027 | BLLAC | 0.527 | 0.151 | 4 | 1,3,4,13 |
| J1758.3+1429 | 269.5800 | 14.4991 | UNCL | 0.152 | - | 1 | 11 |
| J1759.1−4822 | 269.7436 | −48.3535 | UNCL | - | - | - | |
| J1800.1+2812 | 270.0085 | 28.1794 | UNCL | 0.383 | 0.023 | 2 | 4,13 |
| J1800.1+7037 | 269.9542 | 70.6226 | BLLAC | - | - | - | |
| J1800.6+7828 | 270.1903 | 78.4678 | BLLAC | 0.596 | 0.669 | 2 | 3,13 |
| J1801.5+2123 | 270.3520 | 21.3626 | UNCL | - | - | - | |
| J1801.5+4404 | 270.3846 | 44.0728 | FSRQ | 0.329 | 0.274 | 3 | 3,6,13 |
| J1803.4−6510 | 270.8479 | −65.1269 | FSRQ | - | - | - | |
| J1806.2+6143 | 271.5831 | 61.6884 | UNCL | 0.679 | 0.460 | 4 | 3,4,6,13 |
| J1806.3+5345 | 271.6346 | 53.7143 | UNCL | 0.961 | 0.812 | 2 | 3,13 |
| J1806.8+6949 | 271.7112 | 69.8245 | BLLAC | 0.041 | 0.002 | 2 | 5,13 |
| J1806.9−8038 | 271.6785 | −80.7093 | UNCL | - | - | - | |
| J1807.2+6429 | 271.8840 | 64.4906 | BLLAC | 0.197 | 0.045 | 6 | 6,7,8,11,12b,13 |
| J1807.9+4650 | 272.0050 | 46.8280 | BLLAC | 0.441 | 0.446 | 2 | 3,13 |
| J1807.9−6412 | 271.9751 | −64.2306 | FSRQ | 0.234 | - | 1 | 6 |
| J1808.1−5013 | 272.0576 | −50.1982 | FSRQ | - | - | - | |
| J1808.2+3500 | 272.0480 | 35.0219 | UNCL | 0.365 | 0.396 | 2 | 3,13 |
| J1808.8+2419 | 272.1904 | 24.3183 | UNCL | 0.462 | 0.137 | 6 | 4,6,7,8,12b,13 |
| J1808.8+3522 | 272.2071 | 35.3452 | BLLAC | 0.150 | 0.039 | 6 | 4,5,6,11,12b,13 |
| J1809.3+2042 | 272.3560 | 20.6919 | BLLAC | 0.168 | - | 1 | 6 |
| J1809.7+2910 | 272.4391 | 29.1722 | BLLAC | 0.532 | 0.544 | 2 | 3,13 |
| J1810.7+5335 | 272.6583 | 53.5838 | BLLAC | 0.556 | 0.455 | 3 | 3,4,13 |
| J1811.0+1608 | 272.7090 | 16.1391 | BLLAC | 1.362 | 1.165 | 2 | 3,6 |
| J1811.3+0340 | 272.8251 | 3.6871 | UNCL | 0.717 | 0.714 | 2 | 3,6 |
| J1813.5+3144 | 273.3967 | 31.7382 | BLLAC | 0.084 | - | 1 | 13 |
| J1813.6+0614 | 273.3892 | 6.2617 | BLLAC | 0.838 | 0.863 | 2 | 3,6 |
| J1814.0+3828 | 273.5143 | 38.4695 | BLLAC | 0.275 | 0.073 | 4 | 4,6,12b,13 |
| J1814.2+4114 | 273.5946 | 41.2182 | FSRQ | 0.846 | 0.400 | 2 | 3,13 |
| J1814.4+2953 | 273.4053 | 29.8772 | FSRQ | 1.070 | 0.309 | 2 | 3,13 |
| J1816.9−4942 | 274.2333 | −49.7291 | FSRQ | 0.384 | - | 1 | 6 |
| J1818.6+0903 | 274.6669 | 9.0628 | NLS1 | 1.172 | - | 1 | 3 |
| J1819.1+2133 | 274.7717 | 21.5427 | BLLAC | 0.715 | 0.420 | 2 | 3,4 |
| J1820.3+3624 | 275.0874 | 36.3953 | BLLAC | 0.319 | 0.069 | 3 | 4,12b,13 |
| J1821.6+6819 | 275.4979 | 68.3119 | FSRQ | 1.050 | 0.864 | 2 | 3,13 |
| J1822.0+1600 | 275.5415 | 16.0041 | UNCL | 1.129 | - | 1 | 3 |
| J1823.3−3720 | 275.8012 | −37.4010 | UNCL | - | - | - | |
| J1823.5+6858 | 275.8869 | 68.9646 | CLAGN | 0.350 | 0.247 | 2 | 6,13 |
| J1824.1+5651 | 276.0295 | 56.8504 | BLLAC | 0.382 | 0.388 | 2 | 3,13 |
| J1824.5+4311 | 276.0794 | 43.1637 | BLLAC | 0.254 | 0.130 | 4 | 1,6,12b,13 |
| J1825.1−5231 | 276.3075 | −52.5162 | UNCL | - | - | - | |
| J1826.0−5037 | 276.4618 | −50.6543 | UNCL | 0.900 | - | 1 | 4 |
| J1827.6−4029 | 276.8533 | −40.4844 | UNCL | - | - | - | |
| J1828.7+3230 | 277.1479 | 32.5189 | UNCL | - | - | - | |
| J1829.1+2729 | 277.3082 | 27.4841 | UNCL | - | - | - | |
| J1829.2−5813 | 277.3017 | −58.2320 | FSRQ | - | - | - | |
| J1829.3+5402 | 277.3512 | 54.0499 | BLLAC | 0.404 | 0.454 | 2 | 3,13 |
| J1829.5+4845 | 277.3824 | 48.7462 | MIS | 0.409 | 0.437 | 2 | 3,13 |
| J1829.9+3934 | 277.5151 | 39.6106 | UNCL | 0.450 | 0.325 | 3 | 3,4,13 |
| J1830.0+1324 | 277.5032 | 13.4040 | BLLAC | 0.773 | 0.614 | 2 | 3,6 |
| J1830.0−5225 | 277.5180 | −52.4386 | UNCL | - | - | - | |
| J1830.2−4443 | 277.5036 | −44.6866 | UNCL | - | - | - | |
| J1831.9+3820 | 278.0041 | 38.3603 | BLLAC | 0.173 | 0.029 | 6 | 4,5,6,11,12b,13 |
| J1832.6−5658 | 278.1291 | −56.9891 | BLLAC | - | - | - | |
| J1834.2+3136 | 278.5756 | 31.6068 | BLLAC | 0.236 | 0.026 | 2 | 3,6 |
| J1834.7−5858 | 278.6145 | −58.9434 | BLLAC | - | - | - | |
| J1836.4+3137 | 279.0885 | 31.6074 | BLLAC | 0.427 | 0.295 | 2 | 3,6 |
| J1837.0+5347 | 279.2947 | 53.7850 | UNCL | 0.919 | 0.235 | 4 | 3,4,6,13 |
| J1838.0−5959 | 279.5281 | −60.0089 | UNCL | 0.200 | - | 1 | 4 |
| J1838.4−6023 | 279.5860 | −60.4229 | BLLAC | 0.103 | 0.014 | 2 | 5,6 |
| J1838.8+4802 | 279.7048 | 48.0429 | BLLAC | 0.178 | 0.163 | 2 | 4,13 |
| J1838.9−3457 | 279.8482 | −34.8969 | UNCL | 0.454 | - | 1 | 6 |
| J1839.6−7107 | 279.3696 | −71.1454 | FSRQ | - | - | - | |
| J1840.6−5545 | 280.3229 | −55.7381 | UNCL | - | - | - | |
| J1841.0+6115 | 280.1472 | 61.2353 | UNCL | 0.752 | 0.242 | 3 | 3,12b,13 |
| J1841.3+2909 | 280.3405 | 29.1614 | BLLAC | 0.116 | 0.002 | 2 | 5,6 |
| J1841.8+3218 | 280.4460 | 32.3109 | BLLAC | 0.689 | 0.652 | 2 | 3,4 |
| J1842.3+6810 | 280.6402 | 68.1570 | FSRQ | 0.359 | 0.364 | 2 | 3,13 |
| J1842.4+7613 | 280.6068 | 76.1807 | UNCL | 0.344 | 0.107 | 5 | 3,4,6,12b,13 |
| J1842.4−5840 | 280.6242 | −58.6994 | BLLAC | 0.304 | 0.005 | 2 | 4,6 |
| J1843.4−4835 | 280.8109 | −48.6064 | MIS | 0.080 | - | 1 | 6 |
| J1844.9+5709 | 281.2123 | 57.1607 | BLLAC | 0.491 | 0.529 | 2 | 3,13 |
| J1846.7+7238 | 281.5535 | 72.6307 | UNCL | 0.870 | 0.169 | 3 | 3,4,13 |
| J1848.1−4230 | 282.0258 | −42.5075 | UNCL | - | - | - | |
| J1848.4+3217 | 282.0920 | 32.3174 | NLS1 | 1.717 | - | 1 | 3 |
| J1848.5+3243 | 282.1432 | 32.7334 | FSRQ | 0.629 | 0.434 | 2 | 3,6 |
| J1848.5+6537 | 282.0929 | 65.6158 | BLLAC | 0.212 | 0.023 | 2 | 6,12b |
| J1848.6−2711 | 282.1979 | −27.3050 | UNCL | - | - | - | |
| J1848.9+4247 | 282.1962 | 42.7608 | BLLAC | 0.222 | 0.238 | 2 | 4,13 |
| J1849.2+6705 | 282.3170 | 67.0949 | FSRQ | 0.714 | 0.723 | 2 | 3,13 |
| J1849.3−6447 | 282.3601 | −64.8253 | UNCL | 0.243 | - | 1 | 6 |
| J1849.4+2745 | 282.3822 | 27.8002 | BLLAC | 0.739 | 0.425 | 2 | 3,6 |
| J1849.4−4313 | 282.3580 | −43.2370 | BLLAC | - | - | - | |
| J1850.5+2631 | 282.6001 | 26.5316 | AMB | 0.200 | - | 1 | 4 |
| J1851.5+3406 | 282.9217 | 34.1153 | UNCL | 0.876 | 0.452 | 2 | 3,6 |
| J1852.4+4856 | 283.1189 | 48.9299 | FSRQ | 0.666 | 0.046 | 2 | 3,13 |
| J1853.8+6714 | 283.4671 | 67.2319 | BLLAC | 0.185 | 0.026 | 4 | 6,11,12b,13 |
| J1854.6−6007 | 283.7153 | −60.1566 | UNCL | - | - | - | |
| J1855.8−2028 | 283.9812 | −20.4504 | UNCL | - | - | - | |
| J1858.1+7318 | 284.5849 | 73.2870 | UNCL | 0.471 | 0.219 | 3 | 3,4,13 |
| J1858.3+4321 | 284.5560 | 43.4145 | BLLAC | 0.143 | 0.032 | 6 | 4,5,6,11,12b,13 |
| J1858.3−2511 | 284.5795 | −25.1808 | UNCL | 1.289 | - | 1 | 3 |
| J1858.7+5708 | 284.7229 | 57.1360 | SEY | 0.396 | 0.317 | 3 | 3,6,13 |
| J1901.7−5140 | 285.4542 | −51.6522 | UNCL | - | - | - | |
| J1902.9−6748 | 285.7551 | −67.8266 | FSRQ | - | - | - | |
| J1903.2+5540 | 285.7984 | 55.6773 | BLLAC | 0.477 | 0.530 | 2 | 3,13 |
| J1904.1+3627 | 286.0494 | 36.4497 | BLLAC | 0.078 | 0.012 | 3 | 5,6,11 |
| J1906.7+5419 | 286.7393 | 54.3361 | UNCL | - | - | - | |
| J1909.5+3511 | 287.3921 | 35.1804 | UNCL | - | - | - | |
| J1909.7−2140 | 287.4381 | −21.6598 | UNCL | - | - | - | |
| J1910.0−2453 | 287.5646 | −24.7959 | UNCL | 0.334 | - | 1 | 11 |
| J1911.2−2006 | 287.7902 | −20.1153 | FSRQ | - | - | - | |
| J1911.4−1908 | 287.8739 | −19.1402 | BLLAC | 0.136 | 0.035 | 2 | 6,11 |
| J1912.4+3738 | 288.1047 | 37.6768 | FSRQ | 0.731 | 0.597 | 2 | 3,6 |
| J1912.4−1222 | 288.1230 | −12.3836 | UNCL | 1.008 | 1.073 | 2 | 3,6 |
| J1912.7−1250 | 288.2128 | −12.8213 | UNCL | - | - | - | |
| J1913.0−8009 | 288.1667 | −80.1683 | FSRQ | - | - | - | |
| J1913.4−3629 | 288.3370 | −36.5054 | UNCL | 0.600 | - | 1 | 4 |
| J1913.9+4439 | 288.5078 | 44.6423 | BLLAC | 0.943 | 0.858 | 2 | 3,4 |
| J1916.7−1516 | 289.2188 | −15.3167 | UNCL | 0.968 | 0.545 | 2 | 3,6 |
| J1917.7−1921 | 289.4367 | −19.3588 | BLLAC | 0.121 | 0.047 | 2 | 6,11 |
| J1917.7−6442 | 289.3919 | −64.5955 | UNCL | - | - | - | |
| J1917.7−6930 | 289.1512 | −69.4759 | UNCL | - | - | - | |
| J1918.1+3752 | 289.5402 | 37.8870 | UNCL | 0.196 | - | 1 | 6 |
| J1918.2−4111 | 289.5669 | −41.1920 | BLLAC | - | - | - | |
| J1921.3−1231 | 290.3497 | −12.5318 | BLLAC | 0.873 | 0.547 | 2 | 3,6 |
| J1921.7+5817 | 290.4902 | 58.2837 | UNCL | 0.430 | 0.132 | 3 | 4,6,12b |
| J1921.8−1607 | 290.4647 | −16.1202 | BLLAC | - | - | - | |
| J1922.5−7453 | 290.6759 | −74.8991 | UNCL | 0.400 | - | 1 | 4 |
| J1923.4−2503 | 290.8559 | −25.0358 | UNCL | 0.506 | 0.259 | 2 | 4,6 |
| J1923.5−2104 | 290.8841 | −21.0759 | FSRQ | 1.108 | - | 1 | 3 |
| J1924.2−1549 | 291.0493 | −15.8172 | BLLAC | 0.600 | - | 1 | 4 |
| J1924.3−5458 | 291.0427 | −54.9522 | UNCL | 0.300 | - | 1 | 4 |
| J1924.8−2914 | 291.2127 | −29.2417 | FSRQ | 0.740 | - | 1 | 3 |
| J1925.1−1019 | 291.2633 | −10.3034 | UNCL | 1.281 | - | 1 | 3 |
| J1925.1−3358 | 291.3209 | −34.0171 | FSRQ | - | - | - | |
| J1925.8−2220 | 291.4158 | −22.3264 | BLLAC | 1.348 | - | 1 | 3 |
| J1926.8+6154 | 291.7079 | 61.9118 | BLLAC | 0.112 | - | 1 | 13 |
| J1927.5+6117 | 291.8768 | 61.2925 | BLLAC | 0.590 | 0.624 | 2 | 3,13 |
| J1929.4+6146 | 292.3962 | 61.7748 | BLLAC | 0.190 | 0.071 | 4 | 3,4,6,13 |
| J1931.3−1556 | 292.8236 | −15.9647 | UNCL | 0.518 | 0.385 | 2 | 3,6 |
| J1933.2−4539 | 293.1870 | −45.6105 | FSRQ | 0.160 | - | 1 | 6 |
| J1934.2+6002 | 293.5818 | 60.0277 | UNCL | 1.377 | 1.485 | 2 | 3,13 |
| J1934.3+6541 | 293.4889 | 65.6713 | FSRQ | 1.431 | 1.272 | 2 | 3,13 |
| J1934.3−2419 | 293.5532 | −24.3223 | BLLAC | 0.445 | 0.288 | 2 | 3,6 |
| J1934.5+6139 | 293.6695 | 61.6449 | FSRQ | 1.349 | 0.221 | 3 | 1,3,13 |
| J1936.9−4720 | 294.2338 | −47.3306 | BLLAC | 0.155 | - | 1 | 6 |
| J1937.0+8354 | 294.4152 | 83.9414 | UNCL | 1.940 | - | 1 | 3 |
| J1937.2−3958 | 294.3176 | −39.9671 | CLAGN | - | - | - | |
| J1937.2−4217 | 294.3873 | −42.2551 | UNCL | - | - | - | |
| J1939.5−1525 | 294.8611 | −15.4286 | FSRQ | 1.765 | - | 1 | 3 |
| J1939.8−4928 | 294.9420 | −49.4273 | UNCL | 0.314 | - | 1 | 6 |
| J1941.3−6210 | 295.3407 | −62.1892 | BLLAC | 0.588 | - | 1 | 6 |
| J1941.7+7218 | 295.3624 | 72.3617 | UNCL | - | - | - | |
| J1942.5−5827 | 295.6028 | −58.4735 | UNCL | 0.200 | - | 1 | 4 |
| J1942.8−3512 | 295.7779 | −35.1686 | BLLAC | 0.059 | 0.001 | 2 | 5,6 |
| J1944.4−4523 | 296.0933 | −45.3924 | BLLAC | - | - | - | |
| J1944.9−2143 | 296.2299 | −21.7220 | BLLAC | 0.247 | 0.071 | 2 | 4,6 |
| J1945.1−4007 | 296.3310 | −40.0990 | UNCL | 0.600 | - | 1 | 4 |
| J1945.5−0153 | 296.3451 | −1.8894 | UNCL | 1.041 | - | 1 | 3 |
| J1946.0−3112 | 296.4974 | −31.1940 | BLLAC | - | - | - | |
| J1949.5+7311 | 297.5726 | 73.1754 | UNCL | - | - | - | |
| J1951.8−0511 | 297.9478 | −5.1622 | FSRQ | 1.183 | - | 1 | 3 |
| J1953.0+7651 | 298.4620 | 76.8472 | UNCL | 0.765 | 0.417 | 3 | 1,3,4 |
| J1953.0−7025 | 298.2778 | −70.4080 | UNCL | 0.200 | - | 1 | 4 |
| J1954.6−1122 | 298.6715 | −11.3896 | BLLAC | 1.296 | - | 1 | 3 |
| J1954.9−5640 | 298.7619 | −56.6747 | BLLAC | 0.208 | 0.010 | 2 | 4,6 |
| J1955.1−1604 | 298.7528 | −16.0608 | BLLAC | 0.651 | 0.674 | 3 | 3,4,6 |
| J1955.4+5132 | 298.9281 | 51.5302 | FSRQ | 1.294 | - | 1 | 3 |
| J1956.1+0234 | 299.1170 | 2.5737 | UNCL | 1.005 | - | 1 | 3 |
| J1957.1−3231 | 299.2477 | −32.4294 | FSRQ | 0.318 | - | 1 | 6 |
| J1958.0−3845 | 299.4992 | −38.7518 | FSRQ | - | - | - | |
| J1958.1−0711 | 299.5083 | −7.2293 | UNCL | - | - | - | |
| J1958.3−3010 | 299.5621 | −30.1866 | BLLAC | 0.095 | 0.011 | 2 | 5,6 |
| J1959.1−4247 | 299.8053 | −42.7688 | FSRQ | - | - | - | |
| J1959.7−4725 | 299.9403 | −47.4220 | BLLAC | - | - | - | |
| J2000.0+6508 | 299.9994 | 65.1485 | BLLAC | 0.046 | 0.001 | 2 | 5,6 |
| J2000.3−2930 | 300.0707 | −29.5073 | UNCL | 1.366 | - | 1 | 3 |
| J2000.6−1328 | 300.1756 | −13.4260 | FSRQ | 0.214 | 0.083 | 4 | 3,5,6,11 |
| J2000.9−1748 | 300.2379 | −17.8160 | FSRQ | 1.763 | - | 1 | 3 |
| J2001.5−0818 | 300.4177 | −8.3367 | UNCL | 0.417 | 0.270 | 3 | 3,4,6 |
| J2001.7+7040 | 300.3915 | 70.6738 | BLLAC | 0.869 | - | 1 | 3 |
| J2001.9−5737 | 300.5174 | −57.6126 | UNCL | 0.173 | 0.090 | 3 | 2,4,13 |
| J2002.4−7119 | 300.6130 | −71.3280 | BLLAC | - | - | - | |
| J2002.6+6302 | 300.6891 | 63.0426 | BLLAC | 0.787 | 0.477 | 2 | 3,6 |
| J2005.1+7003 | 301.2751 | 70.0776 | UNCL | 2.318 | - | 1 | 3 |
| J2005.2−1822 | 301.3221 | −18.3676 | FSRQ | 0.909 | - | 1 | 3 |
| J2005.5+7752 | 301.3792 | 77.8787 | BLLAC | 0.735 | - | 1 | 3 |
| J2005.8+6424 | 301.5737 | 64.4126 | FSRQ | 1.175 | - | 1 | 3 |
| J2005.9−2309 | 301.4858 | −23.1742 | FSRQ | 0.744 | 0.324 | 2 | 3,6 |
| J2007.2+6607 | 301.8699 | 66.1229 | FSRQ | 1.306 | - | 1 | 3 |
| J2007.3−7728 | 301.7769 | −77.5117 | UNCL | - | - | - | |
| J2007.9−4432 | 301.9799 | −44.5790 | MIS | 0.279 | - | 1 | 6 |
| J2009.4−4849 | 302.3558 | −48.8316 | BLLAC | 0.034 | - | 1 | 6 |
| J2010.0+0726 | 302.4813 | 7.4538 | FSRQ | 0.729 | 0.073 | 2 | 1,3 |
| J2010.0+7229 | 302.4679 | 72.4887 | BLLAC | 0.950 | 0.764 | 2 | 3,6 |
| J2011.6−1546 | 302.8155 | −15.7778 | FSRQ | 1.318 | - | 1 | 3 |
| J2012.2−1646 | 303.1257 | −16.7807 | UNCL | 1.248 | - | 1 | 3 |
| J2013.0−3717 | 303.2019 | −37.3282 | UNCL | 0.600 | - | 1 | 4 |
| J2014.3−0047 | 303.6193 | −0.7897 | BLLAC | 0.274 | 0.168 | 3 | 3,5,6 |
| J2014.5+0648 | 303.6295 | 6.8145 | BLLAC | 0.137 | - | 1 | 6 |
| J2015.0+1621 | 303.7659 | 16.3743 | UNCL | 0.243 | 0.076 | 2 | 4,6 |
| J2015.2−0137 | 303.8132 | −1.6257 | BLLAC | 0.853 | - | 1 | 3 |
| J2015.3−1432 | 303.8543 | −14.5345 | BLLAC | 0.300 | - | 1 | 4 |
| J2015.4+6556 | 303.9807 | 65.9146 | FSRQ | 1.266 | - | 1 | 3 |
| J2016.3−0903 | 304.1002 | −9.0593 | BLLAC | - | - | - | |
| J2016.3−2331 | 303.9989 | −23.5355 | UNCL | - | - | - | |
| J2017.5−3753 | 304.3690 | −37.8961 | BLLAC | 0.451 | - | 1 | 6 |
| J2017.5−4113 | 304.3748 | −41.2544 | BLLAC | 0.242 | - | 1 | 6 |
| J2021.9+0629 | 305.4811 | 6.4871 | BLLAC | 0.473 | 0.353 | 2 | 3,6 |
| J2022.0−7224 | 305.4328 | −72.4366 | UNCL | 0.300 | - | 1 | 4 |
| J2022.3−4513 | 305.6101 | −45.2249 | BLLAC | 0.085 | - | 1 | 13 |
| J2022.5+7612 | 305.6482 | 76.1906 | BLLAC | 0.867 | - | 1 | 3 |
| J2023.6−0123 | 305.8867 | −1.3950 | BLLAC | 0.625 | 0.434 | 2 | 3,4 |
| J2023.6−1139 | 305.9029 | −11.6662 | BLLAC | 0.767 | - | 1 | 11 |
| J2023.8−4828 | 305.9109 | −48.4479 | UNCL | 0.164 | 0.009 | 4 | 6,12a,12b,13 |
| J2024.4−0847 | 306.1224 | −8.8012 | BLLAC | 1.028 | - | 1 | 3 |
| J2024.6−3252 | 306.1482 | −32.8933 | FSRQ | 0.320 | - | 1 | 6 |
| J2024.8−6459 | 306.1932 | −64.9762 | UNCL | 0.624 | 0.131 | 4 | 2,4,6,13 |
| J2025.2+0317 | 306.2901 | 3.2790 | FSRQ | 1.397 | - | 1 | 3 |
| J2025.6−0735 | 306.4194 | −7.5980 | FSRQ | 0.973 | - | 1 | 3 |
| J2026.0−2845 | 306.4734 | −28.7635 | CLAGN | 0.736 | - | 1 | 3 |
| J2026.1+7645 | 306.6283 | 76.7467 | UNCL | 0.258 | 0.095 | 5 | 4,6,7,8,11 |
| J2029.1−1839 | 307.2512 | −18.6194 | UNCL | 0.760 | 0.614 | 2 | 3,4 |
| J2030.2−0620 | 307.5631 | −6.3708 | SEY | 0.644 | 0.039 | 3 | 11,12b,13 |
| J2030.4−0502 | 307.5935 | −5.0535 | FSRQ | 0.416 | 0.207 | 4 | 1,3,6,13 |
| J2030.5−1439 | 307.6163 | −14.6548 | SEY | 0.428 | 0.038 | 3 | 1,4,6 |
| J2030.8−6959 | 307.4740 | −69.9531 | UNCL | - | - | - | |
| J2030.9+1935 | 307.7381 | 19.6036 | BLLAC | 0.235 | 0.086 | 2 | 4,6 |
| J2031.1−2615 | 307.7679 | −26.2588 | UNCL | 0.687 | - | 1 | 3 |
| J2031.2−4121 | 307.7357 | −41.3185 | UNCL | 0.456 | 0.062 | 4 | 6,12a,12b,13 |
| J2031.8+1619 | 307.9254 | 16.3687 | UNCL | 0.149 | 0.042 | 2 | 6,11 |
| J2032.0+1219 | 307.9791 | 12.3282 | FSRQ | 0.704 | 0.438 | 2 | 3,6 |
| J2033.7+6308 | 308.4156 | 63.1445 | UNCL | 0.791 | 0.357 | 2 | 3,6 |
| J2034.6+1154 | 308.6546 | 11.9087 | FSRQ | 0.200 | 0.101 | 2 | 5,6 |
| J2034.8−4200 | 308.7129 | −42.0107 | BLLAC | 0.213 | 0.097 | 5 | 2,4,6,12a,13 |
| J2035.4+1056 | 308.8431 | 10.9352 | FSRQ | - | - | - | |
| J2036.4+6553 | 309.0839 | 65.8874 | BLLAC | 1.066 | - | 1 | 3 |
| J2036.9−3329 | 309.2062 | −33.4752 | BLLAC | 0.296 | - | 1 | 6 |
| J2037.9−0504 | 309.4130 | −5.1394 | UNCL | 0.695 | 0.287 | 3 | 6,11,13 |
| J2039.0−1046 | 309.7530 | −10.7783 | BLLAC | 0.569 | 0.620 | 2 | 3,13 |
| J2039.3+2150 | 309.8950 | 21.8694 | UNCL | 1.976 | 0.902 | 2 | 3,4 |
| J2040.0−5737 | 310.0046 | −57.5860 | UNCL | 0.802 | 0.266 | 3 | 2,12a,13 |
| J2040.1−4621 | 310.0276 | −46.3383 | UNCL | 0.193 | 0.076 | 5 | 4,6,12a,12b,13 |
| J2040.2−2506 | 310.0366 | −25.1296 | FSRQ | 1.583 | - | 1 | 3 |
| J2040.2−7115 | 310.0345 | −71.2500 | AMB | 0.119 | 0.022 | 2 | 5,6 |
| J2040.5−1705 | 310.1156 | −17.1175 | UNCL | 1.890 | 0.225 | 3 | 1,3,4 |
| J2041.8−7319 | 310.5082 | −73.3205 | BLLAC | 0.300 | - | 1 | 4 |
| J2041.9−3735 | 310.4593 | −37.5611 | BLLAC | 0.095 | 0.003 | 2 | 5,6 |
| J2042.1+2427 | 310.5252 | 24.4479 | BLLAC | 0.083 | 0.032 | 3 | 5,6,11 |
| J2042.7−0155 | 310.7029 | −1.8194 | UNCL | 0.888 | 0.281 | 4 | 3,4,6,13 |
| J2042.7−5415 | 310.6785 | −54.1559 | UNCL | 1.518 | 0.909 | 2 | 2,13 |
| J2043.7+0000 | 310.9257 | 0.0219 | UNCL | 0.337 | 0.139 | 3 | 1,4,13 |
| J2044.0+1036 | 310.9652 | 10.5685 | UNCL | 0.259 | - | 1 | 6 |
| J2045.1−2346 | 311.2405 | −23.7790 | UNCL | 0.655 | 0.059 | 2 | 3,4 |
| J2046.6−1012 | 311.7264 | −10.1778 | BLLAC | 0.440 | 0.304 | 4 | 3,4,6,13 |
| J2046.8−4258 | 311.6840 | −42.9535 | BLLAC | 0.461 | - | 1 | 13 |
| J2047.1−7400 | 311.7382 | −74.0011 | FSRQ | - | - | - | |
| J2047.9−3122 | 312.0258 | −31.3378 | UNCL | 0.265 | 0.047 | 2 | 4,6 |
| J2048.6−6804 | 312.1000 | −68.0811 | UNCL | 0.166 | - | 1 | 6 |
| J2049.0+1647 | 312.2625 | 16.7863 | UNCL | 0.686 | 0.394 | 3 | 1,3,4 |
| J2049.7−0036 | 312.3406 | −0.6574 | BLLAC | 0.209 | 0.017 | 3 | 6,12b,13 |
| J2049.9+1002 | 312.4411 | 10.0540 | BLLAC | - | - | - | |
| J2049.9−2453 | 312.5480 | −24.8033 | UNCL | 0.331 | 0.092 | 2 | 4,6 |
| J2050.0+0408 | 312.5260 | 4.1302 | BLLAC | 0.434 | 0.275 | 3 | 1,3,13 |
| J2050.4−2627 | 312.6029 | −26.4717 | FSRQ | 1.109 | - | 1 | 3 |
| J2052.2−5533 | 313.0570 | −55.5528 | FSRQ | 0.507 | 0.076 | 2 | 2,13 |
| J2052.5+0810 | 313.1779 | 8.1772 | BLLAC | - | - | - | |
| J2054.8+0015 | 313.7369 | 0.2605 | BLLAC | 0.127 | 0.026 | 7 | 5,6,7,8,11,12b,13 |
| J2055.4−0020 | 313.8676 | −0.3548 | BLLAC | 0.258 | 0.119 | 2 | 3,13 |
| J2055.4−0504 | 313.8474 | −5.1053 | BLLAC | 0.209 | 0.024 | 6 | 3,6,7,8,12b,13 |
| J2056.2−4714 | 314.0682 | −47.2466 | FSRQ | 0.449 | 0.469 | 2 | 2,13 |
| J2056.4−4904 | 314.0566 | −49.0706 | UNCL | 0.446 | 0.175 | 4 | 2,4,6,13 |
| J2056.5−0202 | 314.1590 | −2.0858 | UNCL | 1.120 | 0.412 | 4 | 1,3,4,13 |
| J2056.7−3209 | 314.1045 | −32.1466 | BLLAC | - | - | - | |
| J2057.4−0723 | 314.3377 | −7.3277 | UNCL | 1.153 | 0.641 | 4 | 1,3,4,13 |
| J2058.8−1442 | 314.6948 | −14.7181 | BLLAC | 0.068 | 0.016 | 3 | 5,6,11 |
| J2100.0+2103 | 315.0211 | 20.9890 | AMB | 0.650 | 0.522 | 2 | 3,6 |
| J2101.3+0912 | 315.3495 | 9.2236 | UNCL | 0.205 | 0.127 | 2 | 4,13 |
| J2101.4−2935 | 315.2569 | −29.5577 | FSRQ | 1.299 | - | 1 | 3 |
| J2103.4−7816 | 316.4375 | −78.4264 | BLLAC | 0.892 | 0.411 | 2 | 4,6 |
| J2103.7−1112 | 315.9450 | −11.2264 | UNCL | - | - | - | |
| J2103.8−6233 | 315.9100 | −62.5405 | BLLAC | 0.176 | 0.166 | 2 | 2,13 |
| J2104.0−3546 | 315.9706 | −35.7723 | UNCL | 0.500 | - | 1 | 4 |
| J2104.3−0212 | 316.0914 | −2.2108 | BLLAC | 1.376 | 1.682 | 2 | 3,13 |
| J2104.7+0108 | 316.1788 | 1.1363 | UNCL | 0.672 | 0.156 | 4 | 1,3,4,13 |
| J2105.2−5143 | 316.3536 | −51.7639 | UNCL | 0.449 | 0.132 | 4 | 2,6,12a,13 |
| J2106.9+2455 | 316.6657 | 25.0160 | UNCL | 0.644 | 0.245 | 3 | 3,4,6 |
| J2107.6−4148 | 316.8466 | −41.7583 | UNCL | 0.694 | 0.075 | 2 | 2,13 |
| J2108.2−2454 | 317.0513 | −24.8759 | UNCL | 1.173 | 0.036 | 2 | 3,4 |
| J2108.3−4824 | 316.9354 | −48.4675 | BLLAC | 0.534 | 0.202 | 3 | 2,4,13 |
| J2108.5+1434 | 317.1710 | 14.5075 | FSRQ | 1.002 | 0.664 | 3 | 3,6,13 |
| J2108.7−0250 | 317.1864 | −2.8428 | BLLAC | 0.076 | 0.025 | 8 | 5,6,7,8,9,11,12b,13 |
| J2108.9−6638 | 317.2159 | −66.6230 | BLLAC | - | - | - | |
| J2109.6+0440 | 317.4172 | 4.6668 | BLLAC | 0.276 | 0.192 | 2 | 1,13 |
| J2109.8−8618 | 317.5466 | −86.3132 | UNCL | 0.395 | 0.126 | 2 | 4,6 |
| J2110.2−1021c | 317.5041 | −10.3493 | FSRQ | 1.294 | 1.135 | 4 | 3,4,6,13 |
| J2110.3+0808 | 317.5403 | 8.1654 | FSRQ | 1.113 | 0.310 | 3 | 1,3,13 |
| J2112.7+0819 | 318.1792 | 8.3098 | BLLAC | 0.393 | 0.248 | 3 | 3,4,13 |
| J2114.7+3130 | 318.7102 | 31.5059 | UNCL | 0.950 | - | 1 | 11 |
| J2114.8+2026 | 318.7204 | 20.4408 | UNCL | 0.211 | 0.032 | 6 | 3,4,6,7,8,11 |
| J2114.8+2831 | 318.7431 | 28.5492 | FSRQ | 2.318 | - | 1 | 3 |
| J2115.4+2932 | 318.8726 | 29.5607 | FSRQ | 1.064 | - | 1 | 3 |
| J2115.6−4938 | 318.9371 | −49.6519 | UNCL | 0.285 | - | 1 | 6 |
| J2115.8+6753 | 319.0741 | 67.8900 | UNCL | 0.409 | 0.011 | 2 | 4,11 |
| J2115.9−0113 | 319.0135 | −1.1412 | BLLAC | 0.166 | 0.084 | 8 | 2,3,6,8,11,12a,12b,13 |
| J2116.2+3339 | 319.0605 | 33.6557 | BLLAC | - | - | - | |
| J2116.3+1015 | 318.9601 | 10.2590 | UNCL | 1.012 | - | 1 | 13 |
| J2117.8−1521 | 319.4648 | −15.3783 | UNCL | 2.300 | - | 1 | 4 |
| J2117.8−3243 | 319.4788 | −32.7245 | BLLAC | 0.204 | 0.002 | 2 | 5,6 |
| J2118.0+0019 | 319.5725 | 0.2213 | SEY | 0.584 | 0.167 | 4 | 1,2,3,13 |
| J2118.8−0723c | 319.7207 | −7.5410 | SEY | 0.203 | 0.040 | 5 | 3,6,9,12b,13 |
| J2119.0−3317 | 319.7219 | −33.2808 | UNCL | - | - | - | |
| J2119.6−1105 | 319.9162 | −11.1041 | FSRQ | 1.051 | 0.250 | 2 | 3,13 |
| J2120.6−1254 | 320.1486 | −12.9114 | SEY | 0.484 | 0.066 | 4 | 6,11,12b,13 |
| J2120.6−6114 | 320.2670 | −61.1902 | FSRQ | 0.516 | 0.646 | 2 | 2,13 |
| J2121.0+1901 | 320.2525 | 19.0245 | FSRQ | 1.233 | 0.261 | 3 | 1,3,13 |
| J2123.6+0535 | 320.9355 | 5.5895 | FSRQ | 0.730 | 0.338 | 2 | 3,13 |
| J2123.8−3148 | 320.9367 | −31.9338 | UNCL | - | - | - | |
| J2126.1−3922 | 321.6050 | −39.3562 | BLLAC | 0.500 | - | 1 | 4 |
| J2126.3−4605 | 321.6279 | −46.0966 | UNCL | 0.612 | 0.784 | 2 | 2,13 |
| J2126.5+1842 | 321.6186 | 18.6837 | UNCL | 0.851 | 0.540 | 3 | 3,4,13 |
| J2127.6−5959 | 321.8743 | −60.0175 | AMB | 0.928 | 1.448 | 3 | 4,12a,13 |
| J2127.7+3612 | 321.9293 | 36.2183 | BLLAC | 0.590 | 0.541 | 2 | 3,6 |
| J2130.2−7320 | 322.6609 | −73.4178 | BLLAC | 0.044 | 0.000 | 2 | 5,6 |
| J2130.4−4241 | 322.5684 | −42.7287 | UNCL | 0.148 | 0.007 | 5 | 5,6,12a,12b,13 |
| J2130.8−6623 | 322.6613 | −66.3990 | UNCL | - | - | - | |
| J2131.0−2746 | 322.7635 | −27.7828 | BLLAC | - | - | - | |
| J2131.5−0916 | 322.8976 | −9.2566 | BLLAC | 0.693 | 0.786 | 3 | 3,6,13 |
| J2131.7−2515 | 322.9648 | −25.2663 | BLLAC | - | - | - | |
| J2132.0−5418 | 323.0346 | −54.3435 | UNCL | 0.705 | 0.273 | 2 | 2,13 |
| J2133.0+2610 | 323.2210 | 26.1955 | UNCL | 1.115 | 0.026 | 2 | 1,3 |
| J2133.1+2529c | 323.3098 | 25.4831 | BLLAC | 0.207 | 0.050 | 4 | 3,6,7,8 |
| J2133.6+1439 | 323.4058 | 14.7296 | UNCL | 0.676 | 0.457 | 4 | 3,4,6,13 |
| J2133.9+6646 | 323.4548 | 66.7846 | UNCL | 0.699 | 0.483 | 2 | 3,6 |
| J2134.2−0154 | 323.5430 | −1.8881 | CLAGN | 0.427 | 0.449 | 2 | 3,13 |
| J2134.3−6511 | 323.5551 | −65.2270 | UNCL | 0.632 | 0.177 | 2 | 2,13 |
| J2134.5−2130 | 323.6257 | −21.5091 | BLLAC | 0.501 | 0.398 | 2 | 3,6 |
| J2135.3−5006 | 323.8340 | −50.1144 | FSRQ | 1.516 | 0.846 | 2 | 2,13 |
| J2136.2+0032 | 324.1608 | 0.6984 | FSRQ | 1.268 | 0.837 | 3 | 2,3,13 |
| J2136.2−0642 | 324.0930 | −6.7311 | FSRQ | 0.780 | 0.433 | 3 | 1,3,13 |
| J2138.3+3556 | 324.5281 | 35.9082 | UNCL | 0.629 | 0.439 | 2 | 3,4 |
| J2138.8−2055 | 324.7198 | −20.8966 | BLLAC | 0.547 | 0.299 | 2 | 3,6 |
| J2139.2−2214 | 324.8113 | −22.2196 | UNCL | 1.437 | 0.716 | 2 | 3,4 |
| J2139.4−4235 | 324.8507 | −42.5890 | BLLAC | 0.468 | 0.624 | 3 | 2,12a,13 |
| J2139.9+3910 | 325.0706 | 39.1958 | UNCL | - | - | - | |
| J2140.5−6731 | 324.8050 | −67.5355 | FSRQ | - | - | - | |
| J2141.7−6410 | 325.4435 | −64.1874 | FSRQ | 0.416 | 0.347 | 3 | 2,6,13 |
| J2141.8−3727 | 325.4685 | −37.4869 | FSRQ | - | - | - | |
| J2142.4+3659 | 325.6104 | 36.9971 | UNCL | 0.156 | 0.058 | 2 | 4,6 |
| J2142.5−2552 | 325.5664 | −25.8574 | UNCL | 1.367 | - | 1 | 3 |
| J2142.7−0437 | 325.6538 | −4.6288 | FSRQ | 0.161 | 0.031 | 3 | 3,6,13 |
| J2142.8+1958 | 325.6979 | 19.9697 | UNCL | 0.760 | 0.814 | 4 | 1,4,6,13 |
| J2143.0−5501 | 325.4346 | −55.1583 | FSRQ | 0.152 | 0.015 | 3 | 2,6,13 |
| J2143.1−3929 | 325.7619 | −39.4903 | BLLAC | 0.279 | 0.162 | 2 | 6,13 |
| J2143.5+1743 | 325.8981 | 17.7302 | FSRQ | 0.222 | 0.185 | 3 | 3,6,13 |
| J2143.9+3337 | 325.9589 | 33.6197 | UNCL | - | - | - | |
| J2144.2+3132 | 326.0634 | 31.5609 | BLLAC | 0.623 | - | 1 | 3 |
| J2144.3−7802 | 326.6253 | −77.9319 | FSRQ | 0.321 | - | 1 | 6 |
| J2144.8−1817 | 326.1754 | −18.3001 | UNCL | 0.159 | 0.029 | 3 | 4,6,11 |
| J2145.0−3356 | 326.2547 | −33.9546 | FSRQ | - | - | - | |
| J2145.5+1006 | 326.3758 | 10.1015 | BLLAC | 0.499 | 0.108 | 4 | 1,3,4,13 |
| J2145.7+0718 | 326.4679 | 7.3242 | BLLAC | 0.183 | 0.045 | 6 | 6,7,8,9,12b,13 |
| J2146.4−1528 | 326.5957 | −15.4289 | FSRQ | 0.850 | - | 1 | 3 |
| J2146.5−1344 | 326.6540 | −13.7335 | BLLAC | 0.481 | 0.496 | 2 | 3,13 |
| J2146.8+0425 | 326.7300 | 4.4571 | UNCL | 1.181 | 0.577 | 5 | 1,3,4,6,13 |
| J2147.1+0931 | 326.7923 | 9.4963 | FSRQ | 0.462 | 0.419 | 2 | 3,13 |
| J2147.3−7536 | 326.8030 | −75.6037 | FSRQ | - | - | - | |
| J2148.0−0733 | 327.0294 | −7.5630 | AMB | 0.303 | 0.149 | 3 | 1,6,13 |
| J2148.6+0652 | 327.0227 | 6.9607 | FSRQ | 0.559 | 0.713 | 2 | 3,13 |
| J2148.9−0121 | 327.1808 | −1.3773 | SEY | 0.184 | 0.015 | 9 | 5,6,7,8,9,11,12a,12b,13 |
| J2149.6+0323 | 327.4245 | 3.3810 | BLLAC | 0.364 | 0.345 | 2 | 3,13 |
| J2149.7+1917 | 327.4469 | 19.3462 | UNCL | 1.347 | 0.592 | 3 | 1,3,13 |
| J2150.1−1410 | 327.5647 | −14.1805 | BLLAC | 0.146 | 0.030 | 5 | 5,6,11,12b,13 |
| J2150.7−1750 | 327.6942 | −17.8317 | BLLAC | 0.192 | - | 1 | 6 |
| J2150.7−2810 | 327.7212 | −28.2116 | FSRQ | 0.854 | - | 1 | 3 |
| J2150.8+1118 | 327.7158 | 11.3211 | BLLAC | 0.326 | 0.097 | 3 | 1,6,13 |
| J2151.7−2749 | 327.8415 | −27.7065 | FSRQ | 0.933 | - | 1 | 3 |
| J2151.8−3027 | 327.9813 | −30.4649 | FSRQ | - | - | - | |
| J2152.0−1205 | 328.0588 | −12.0949 | BLLAC | 0.641 | 0.694 | 2 | 3,13 |
| J2152.5+1737 | 328.1034 | 17.5772 | BLLAC | 0.626 | 0.269 | 3 | 1,3,13 |
| J2153.1−0041 | 328.2723 | −0.7085 | BLLAC | 0.177 | 0.039 | 6 | 2,6,8,12a,12b,13 |
| J2153.8−1137 | 328.4593 | −11.6039 | UNCL | 0.703 | 0.258 | 3 | 3,6,13 |
| J2156.0+1818 | 329.0068 | 18.3103 | BLLAC | 1.359 | 1.672 | 2 | 3,13 |
| J2156.0−6942 | 329.2749 | −69.6899 | MIS | 0.017 | - | 1 | 5 |
| J2156.3−0036 | 329.0615 | −0.6179 | BLLAC | 0.852 | 0.308 | 4 | 1,2,3,13 |
| J2156.9−0854 | 329.2097 | −8.9265 | BLLAC | 0.577 | 0.354 | 3 | 1,3,13 |
| J2157.5+3127 | 329.3701 | 31.4504 | FSRQ | 0.842 | - | 1 | 3 |
| J2158.1−1501 | 329.5262 | −15.0193 | CLAGN | 0.484 | 0.514 | 2 | 3,13 |
| J2158.8−3013 | 329.7169 | −30.2256 | BLLAC | 0.030 | - | 1 | 6 |
| J2159.1−2840 | 329.7955 | −28.6879 | BLLAC | 0.185 | - | 1 | 6 |
| J2159.8−4751 | 329.9963 | −47.8665 | UNCL | 0.582 | 0.509 | 2 | 2,13 |
| J2200.1+2138 | 330.0592 | 21.6325 | BLLAC | 0.470 | 0.303 | 3 | 1,3,13 |
| J2200.3+1029 | 330.0331 | 10.5022 | BLLAC | 0.845 | 0.266 | 3 | 1,3,13 |
| J2200.7−2414 | 330.1528 | −24.2410 | UNCL | 0.620 | 0.294 | 2 | 3,4 |
| J2201.0−5907 | 330.2805 | −59.1113 | UNCL | 0.122 | 0.046 | 5 | 4,5,6,12a,13 |
| J2201.5+2950 | 330.3492 | 29.8263 | BLLAC | 0.118 | 0.033 | 2 | 6,11 |
| J2201.5−8339 | 330.5802 | −83.6366 | FSRQ | - | - | - | |
| J2201.9−1706 | 330.4826 | −17.1168 | BLLAC | 0.145 | 0.013 | 3 | 5,6,11 |
| J2202.7+4216 | 330.6804 | 42.2778 | BLLAC | 0.067 | - | 1 | 6 |
| J2202.7−5637 | 330.7221 | −56.5953 | MIS | 0.058 | 0.012 | 4 | 5,6,12a,13 |
| J2203.4+1725 | 330.8621 | 17.4301 | FSRQ | 0.762 | 0.396 | 3 | 3,6,13 |
| J2204.3+0438 | 331.0736 | 4.6672 | SEY | 0.029 | 0.005 | 5 | 5,6,9,11,13 |
| J2204.5+3634 | 331.0879 | 36.5436 | BLLAC | 0.068 | 0.002 | 3 | 5,6,11 |
| J2205.0+7432 | 331.4474 | 74.6059 | UNCL | 1.382 | - | 1 | 3 |
| J2206.8−0032 | 331.6803 | −0.5174 | BLLAC | 0.837 | 0.237 | 4 | 1,2,3,13 |
| J2207.0+3607 | 331.7854 | 36.1597 | UNCL | - | - | - | |
| J2207.1+4316 | 331.7897 | 43.2743 | UNCL | 1.645 | - | 1 | 3 |
| J2207.5−5346 | 331.9322 | −53.7761 | FSRQ | 0.634 | 0.821 | 2 | 2,13 |
| J2207.6+0053 | 331.9085 | 0.8758 | CLAGN | 1.170 | 0.740 | 4 | 1,2,3,13 |
| J2208.1−4507 | 332.0368 | −45.1554 | UNCL | 0.524 | 0.346 | 2 | 6,13 |
| J2209.4+4329 | 332.3646 | 43.4803 | UNCL | 0.618 | 0.305 | 3 | 1,3,6 |
| J2209.7−0451 | 332.4237 | −4.8529 | BLLAC | 0.310 | 0.123 | 4 | 1,3,6,13 |
| J2209.8−5028 | 332.5667 | −50.5182 | UNCL | 0.900 | 0.866 | 2 | 2,13 |
| J2210.8+3203 | 332.7439 | 32.0614 | UNCL | 0.220 | 0.057 | 3 | 4,6,11 |
| J2211.0−0003 | 332.7848 | −0.0507 | BLLAC | 0.278 | 0.088 | 5 | 2,7,8,9,13 |
| J2211.2−1325 | 332.8504 | −13.4694 | FSRQ | 0.436 | 0.540 | 2 | 3,13 |
| J2211.4−7040 | 332.9843 | −70.6541 | UNCL | 0.200 | - | 1 | 4 |
| J2212.0+2356 | 333.0249 | 23.9279 | CLAGN | 0.759 | 0.196 | 3 | 1,3,13 |
| J2212.2−7251 | 332.8471 | −72.8187 | UNCL | 0.280 | - | 1 | 6 |
| J2212.6+2800 | 333.1629 | 27.9940 | BLLAC | 0.499 | 0.204 | 4 | 1,3,6,13 |
| J2212.8+0647 | 333.2118 | 6.7691 | FSRQ | 0.972 | 0.206 | 3 | 1,3,13 |
| J2212.9−2526 | 333.2604 | −25.4917 | FSRQ | 0.728 | 0.384 | 2 | 3,6 |
| J2213.5−4754 | 333.3765 | −47.9070 | BLLAC | 0.378 | 0.104 | 2 | 2,13 |
| J2216.8+3103 | 334.1780 | 31.0432 | FSRQ | 1.462 | 0.690 | 2 | 1,13 |
| J2216.9+2421 | 334.2534 | 24.3628 | BLLAC | 0.517 | 0.221 | 3 | 3,6,13 |
| J2218.6+1941 | 334.7274 | 19.6448 | UNCL | 0.690 | 0.344 | 6 | 3,4,7,8,9,13 |
| J2219.2+1806 | 334.8087 | 18.1099 | FSRQ | 1.177 | 0.258 | 2 | 3,13 |
| J2219.2−0342 | 334.7168 | −3.5936 | FSRQ | 1.355 | 1.731 | 2 | 3,13 |
| J2220.5+2813 | 335.1197 | 28.2321 | BLLAC | 0.128 | 0.035 | 8 | 5,6,7,8,9,11,12b,13 |
| J2221.5−5225 | 335.3721 | −52.4244 | BLLAC | 0.748 | 0.921 | 3 | 2,6,13 |
| J2221.9−3504 | 335.6128 | −35.1639 | UNCL | - | - | - | |
| J2222.8+1209 | 335.7208 | 12.2305 | FSRQ | 0.849 | 0.280 | 3 | 1,3,13 |
| J2223.3+0102 | 335.8732 | 1.0407 | BLLAC | 0.616 | 0.306 | 4 | 1,2,3,13 |
| J2224.0−1127 | 336.0332 | −11.4392 | BLLAC | 0.748 | 0.149 | 2 | 3,13 |
| J2224.3+7737 | 336.8401 | 77.5553 | UNCL | 0.100 | - | 1 | 4 |
| J2224.5+0353 | 336.1041 | 3.9162 | SEY | 0.481 | 0.346 | 5 | 1,3,4,12b,13 |
| J2225.5−1114 | 336.4322 | −11.2280 | BLLAC | 0.736 | 0.464 | 2 | 3,13 |
| J2225.6+2120 | 336.4085 | 21.3018 | FSRQ | 1.141 | 1.412 | 2 | 3,13 |
| J2225.7−0457 | 336.4469 | −4.9504 | CLAGN | 0.401 | 0.330 | 2 | 3,13 |
| J2226.6+0210 | 336.6518 | 2.1770 | BLLAC | 0.313 | 0.110 | 8 | 4,6,7,8,9,12b,12c,13 |
| J2226.8+0051 | 336.6939 | 0.8698 | FSRQ | 0.791 | 0.279 | 7 | 2,3,6,7,8,9,13 |
| J2227.9+0036 | 336.9922 | 0.6182 | BLLAC | 0.503 | 0.493 | 3 | 2,3,13 |
| J2227.9−3031 | 336.9610 | −30.5621 | MIS | 0.074 | 0.003 | 2 | 5,6 |
| J2228.0−4155 | 336.9967 | −41.9524 | BLLAC | - | - | - | |
| J2228.6−1636 | 337.1258 | −16.6120 | BLLAC | 0.888 | - | 1 | 3 |
| J2229.1+2254 | 337.3096 | 22.9194 | BLLAC | 0.449 | 0.024 | 8 | 4,6,7,8,9,11,12b,13 |
| J2229.2−6911 | 337.2507 | −69.1751 | FSRQ | - | - | - | |
| J2229.7−0832 | 337.4170 | −8.5485 | FSRQ | 0.554 | 0.568 | 2 | 3,13 |
| J2230.9−7815 | 337.6273 | −78.2657 | FSRQ | - | - | - | |
| J2231.0−4416 | 337.7352 | −44.2750 | FSRQ | 0.440 | 0.053 | 2 | 2,13 |
| J2232.6+1143 | 338.1517 | 11.7308 | FSRQ | 0.614 | 0.656 | 2 | 3,13 |
| J2232.6−2023 | 338.2033 | −20.3739 | BLLAC | - | - | - | |
| J2232.8+1334 | 338.2547 | 13.6006 | BLLAC | 0.173 | 0.047 | 7 | 6,7,8,9,11,12b,13 |
| J2233.9−1229 | 338.4789 | −12.5095 | UNCL | 0.181 | 0.017 | 5 | 5,6,11,12b,13 |
| J2234.1−2656 | 338.5350 | −26.9457 | UNCL | 0.252 | - | 1 | 3 |
| J2235.1−0623 | 338.7629 | −6.3836 | UNCL | 0.520 | 0.162 | 7 | 3,4,6,7,8,9,13 |
| J2235.3−4836 | 338.8052 | −48.5997 | FSRQ | 0.328 | 0.334 | 3 | 2,12a,13 |
| J2235.8−3627 | 338.9785 | −36.4841 | BLLAC | 0.442 | - | 1 | 6 |
| J2236.2−1706 | 339.0397 | −17.1061 | BLLAC | 0.487 | 0.256 | 2 | 3,6 |
| J2236.3+2828 | 339.0936 | 28.4826 | CLAGN | 0.913 | 1.040 | 2 | 3,13 |
| J2236.4−2309 | 339.1093 | −23.1574 | UNCL | - | - | - | |
| J2236.5−1433 | 339.1420 | −14.5562 | BLLAC | 1.516 | - | 1 | 3 |
| J2236.6+3706 | 339.1098 | 37.1204 | BLLAC | 0.161 | 0.034 | 5 | 5,6,7,8,11 |
| J2237.0−3921 | 339.2838 | −39.3606 | FSRQ | 0.300 | 0.013 | 3 | 6,12b,13 |
| J2239.2−5657 | 339.8003 | −57.0169 | FSRQ | 1.241 | 0.346 | 2 | 2,13 |
| J2240.3−1246 | 340.0630 | −12.7941 | UNCL | 0.167 | 0.040 | 4 | 6,11,12b,13 |
| J2240.7−4746 | 340.1754 | −47.7927 | UNCL | 0.134 | - | 1 | 5 |
| J2241.1−4122 | 340.2613 | −41.3653 | UNCL | 1.150 | - | 1 | 13 |
| J2241.2+4120 | 340.2800 | 41.3366 | BLLAC | 0.726 | - | 1 | 3 |
| J2241.3+2943 | 340.3481 | 29.7132 | BLLAC | 0.400 | 0.127 | 4 | 1,4,6,13 |
| J2243.4−2544 | 340.8600 | −25.7419 | BLLAC | 1.044 | - | 1 | 3 |
| J2243.5−3931 | 340.8587 | −39.5647 | UNCL | 1.202 | - | 1 | 13 |
| J2243.7−1231 | 340.9181 | −12.5166 | BLLAC | 0.213 | - | 1 | 13 |
| J2243.8−2510 | 340.9182 | −25.0998 | UNCL | 1.623 | 0.903 | 2 | 3,4 |
| J2243.9+2021 | 340.9781 | 20.3510 | BLLAC | 0.028 | - | 1 | 13 |
| J2244.2+4057 | 341.0530 | 40.9538 | FSRQ | 0.752 | 0.298 | 2 | 3,6 |
| J2244.9−0007 | 341.2004 | −0.1054 | BLLAC | 0.818 | 0.716 | 5 | 1,2,3,12c,13 |
| J2245.5−1734 | 341.3830 | −17.5661 | UNCL | 0.653 | 0.323 | 3 | 1,3,4 |
| J2245.9+1544 | 341.5208 | 15.7432 | BLLAC | 0.404 | 0.167 | 3 | 1,3,13 |
| J2246.7−5207 | 341.6754 | −52.1112 | BLLAC | 0.133 | 0.039 | 4 | 6,12a,12b,13 |
| J2247.4−0001 | 341.8758 | 0.0018 | BLLAC | 0.639 | 0.369 | 4 | 1,2,3,13 |
| J2247.5−3700 | 341.7659 | −36.9629 | FSRQ | - | - | - | |
| J2247.8+4413 | 341.9717 | 44.2209 | BLLAC | 1.899 | - | 1 | 3 |
| J2248.7−3235 | 342.1612 | −32.5978 | FSRQ | - | - | - | |
| J2248.9+2106 | 342.2524 | 21.1175 | FSRQ | 1.224 | 0.683 | 3 | 1,3,13 |
| J2249.4−1300 | 342.2946 | −13.0006 | BLLAC | 0.259 | 0.174 | 3 | 4,6,13 |
| J2249.7−5944 | 342.4102 | −59.7397 | UNCL | 0.242 | 0.091 | 6 | 2,4,6,12a,12b,13 |
| J2249.9+0452 | 342.5306 | 4.9382 | UNCL | 0.763 | 0.080 | 7 | 3,7,8,9,12b,12c,13 |
| J2250.0+3825 | 342.5240 | 38.4103 | BLLAC | 0.075 | 0.010 | 2 | 5,6 |
| J2250.0−1250 | 342.4984 | −12.8547 | UNCL | 0.600 | 0.761 | 2 | 3,13 |
| J2250.4+1748 | 342.6365 | 17.8208 | BLLAC | 0.278 | 0.053 | 7 | 6,7,8,9,11,12b,13 |
| J2250.4−4206 | 342.5926 | −42.1037 | UNCL | 0.290 | 0.214 | 2 | 2,13 |
| J2250.7−2806 | 342.6854 | −28.1109 | BLLAC | 1.642 | - | 1 | 3 |
| J2251.5−4928 | 342.8696 | −49.4864 | UNCL | 0.143 | 0.010 | 2 | 2,13 |
| J2251.7−3208 | 342.9480 | −32.1036 | BLLAC | - | - | - | |
| J2252.0+4031 | 342.9990 | 40.5162 | BLLAC | 0.135 | - | 1 | 6 |
| J2252.6+1245 | 343.1341 | 12.7530 | BLLAC | 0.345 | 0.149 | 3 | 1,3,13 |
| J2253.2−1232 | 343.3449 | −12.5315 | UNCL | 0.822 | - | 1 | 13 |
| J2253.3+3233 | 343.3021 | 32.6012 | FSRQ | 0.263 | 0.090 | 3 | 3,6,13 |
| J2253.7+1405 | 343.4760 | 14.0769 | BLLAC | 0.191 | 0.052 | 6 | 6,7,8,9,12b,13 |
| J2253.9+1609 | 343.4906 | 16.1482 | FSRQ | 0.579 | 0.740 | 2 | 3,13 |
| J2254.2+4305 | 343.4840 | 43.0754 | UNCL | 0.106 | 0.007 | 2 | 4,11 |
| J2254.8−2725 | 343.7217 | −27.4191 | BLLAC | 0.248 | 0.021 | 2 | 3,6 |
| J2255.2+2411 | 343.8141 | 24.1698 | BLLAC | 0.547 | 0.700 | 2 | 3,13 |
| J2256.0−2740 | 344.0006 | −27.5989 | FSRQ | 1.821 | - | 1 | 3 |
| J2256.4−7119 | 344.0368 | −71.2607 | UNCL | - | - | - | |
| J2256.6−2011 | 344.1717 | −20.1946 | BLLAC | 0.858 | - | 1 | 3 |
| J2256.7+1307 | 344.1011 | 13.0949 | BLLAC | 0.513 | 0.216 | 4 | 1,3,6,13 |
| J2257.5+0748 | 344.3221 | 7.7201 | BLLAC | 0.165 | 0.091 | 4 | 3,6,11,13 |
| J2258.1−2759 | 344.5248 | −27.9726 | FSRQ | 0.808 | - | 1 | 3 |
| J2258.3−3643 | 344.5626 | −36.7429 | BLLAC | 0.319 | - | 1 | 6 |
| J2258.4−5524 | 344.5791 | −55.4271 | BLLAC | 0.196 | 0.079 | 3 | 2,6,13 |
| J2258.5−8247 | 344.4975 | −82.7814 | UNCL | 0.252 | 0.064 | 2 | 4,6 |
| J2259.7−3549 | 344.9243 | −35.8130 | UNCL | - | - | - | |
| J2259.8−1552 | 344.9886 | −15.8926 | UNCL | 1.625 | 0.634 | 2 | 3,4 |
| J2300.1+4053 | 345.0515 | 40.8736 | BLLAC | 0.238 | 0.083 | 2 | 4,6 |
| J2300.3+3136 | 345.0952 | 31.6179 | BLLAC | 0.502 | 0.518 | 2 | 3,13 |
| J2300.7−2645 | 345.1063 | −26.7397 | FSRQ | 1.235 | - | 1 | 3 |
| J2300.9+7108 | 345.2093 | 71.1705 | UNCL | 1.747 | - | 1 | 3 |
| J2301.0−0158 | 345.2832 | −1.9679 | FSRQ | 0.648 | 0.196 | 3 | 1,3,13 |
| J2302.8−1841 | 345.7624 | −18.6905 | MIS | 0.289 | 0.187 | 3 | 3,5,6 |
| J2304.3+0618 | 346.1179 | 6.3356 | FSRQ | 0.776 | 0.532 | 4 | 1,3,6,13 |
| J2304.6+3704 | 346.1530 | 37.0854 | BLLAC | - | - | - | |
| J2306.6−1105 | 346.6479 | −11.0637 | UNCL | 0.640 | 0.044 | 3 | 11,12b,13 |
| J2307.4−1206 | 346.8421 | −12.0882 | BLLAC | 0.681 | 0.222 | 2 | 3,13 |
| J2307.6+1451 | 346.8917 | 14.8383 | BLLAC | 0.555 | 0.168 | 4 | 1,3,6,13 |
| J2308.9+1111 | 347.2159 | 11.1971 | UNCL | 0.824 | 0.469 | 3 | 3,4,13 |
| J2309.7−3632 | 347.4202 | −36.5469 | BLLAC | - | - | - | |
| J2311.0+0205 | 347.7554 | 2.0848 | BLLAC | 0.497 | 0.355 | 3 | 2,3,13 |
| J2311.0+3425 | 347.7722 | 34.4197 | FSRQ | 0.604 | 0.225 | 2 | 1,3 |
| J2311.7+2604 | 347.9412 | 26.0799 | FSRQ | 0.791 | 0.392 | 3 | 1,3,13 |
| J2311.8+4541 | 347.9475 | 45.7322 | FSRQ | 1.529 | - | 1 | 3 |
| J2312.5+7241 | 348.0821 | 72.6908 | UNCL | 2.024 | - | 1 | 3 |
| J2313.4−6922 | 348.4495 | −69.3919 | UNCL | 0.500 | - | 1 | 4 |
| J2313.5+3945 | 348.3514 | 39.8305 | UNCL | 1.195 | 0.406 | 2 | 3,4 |
| J2313.9−4501 | 348.5391 | −44.9303 | FSRQ | 1.056 | 0.658 | 2 | 2,13 |
| J2314.0+1445 | 348.4889 | 14.7398 | BLLAC | 0.124 | 0.018 | 8 | 5,6,7,8,9,11,12b,13 |
| J2315.6−5018 | 348.9347 | −50.3110 | BLLAC | 1.144 | 0.788 | 3 | 2,6,13 |
| J2316.9−5210 | 349.2572 | −52.1671 | BLLAC | 0.247 | 0.075 | 3 | 2,4,13 |
| J2317.0+3756 | 349.2928 | 37.9967 | UNCL | 1.105 | - | 1 | 3 |
| J2317.4−4533 | 349.3833 | −45.5666 | BLLAC | 0.150 | - | 1 | 13 |
| J2318.2+1915 | 349.5955 | 19.2478 | FSRQ | 1.353 | 0.608 | 2 | 1,13 |
| J2319.1−4207 | 349.7746 | −42.1134 | BLLAC | 0.043 | 0.015 | 5 | 5,6,12a,12b,13 |
| J2319.7+1609 | 349.9310 | 16.1973 | BLLAC | 0.152 | 0.017 | 2 | 6,13 |
| J2320.8−0823 | 350.3260 | −8.4560 | FSRQ | 1.950 | 1.504 | 2 | 1,13 |
| J2321.0−6308 | 350.1660 | −63.1550 | BLLAC | 0.175 | 0.035 | 3 | 2,4,13 |
| J2321.5−1619 | 350.4042 | −16.3246 | BLLAC | - | - | - | |
| J2321.7−6438 | 350.4259 | −64.6353 | BLLAC | 0.170 | 0.107 | 2 | 2,13 |
| J2321.9+2734 | 350.4994 | 27.5462 | FSRQ | 0.503 | 0.454 | 3 | 3,6,13 |
| J2321.9+3204 | 350.4790 | 32.0688 | FSRQ | 0.903 | 0.391 | 3 | 3,6,13 |
| J2322.1+4440 | 350.5848 | 44.7618 | BLLAC | 1.227 | - | 1 | 3 |
| J2322.6−0735 | 350.7170 | −7.6182 | UNCL | 0.686 | 0.358 | 4 | 1,3,4,13 |
| J2322.7+3436 | 350.6834 | 34.6039 | BLLAC | 0.070 | 0.015 | 8 | 5,6,7,8,9,11,12b,13 |
| J2322.8−4916 | 350.7268 | −49.2750 | BLLAC | 0.372 | 0.371 | 2 | 2,13 |
| J2323.5−0317 | 350.8831 | −3.2847 | FSRQ | 0.568 | 0.325 | 3 | 1,3,13 |
| J2323.6−0617 | 350.9130 | −6.2998 | FSRQ | 1.267 | 0.723 | 4 | 1,3,12b,13 |
| J2323.8+4210 | 350.9670 | 42.1829 | BLLAC | - | - | - | |
| J2324.7+0801 | 351.1889 | 8.0350 | BLLAC | 0.650 | 0.827 | 2 | 3,13 |
| J2324.7−4041 | 351.1861 | −40.6804 | BLLAC | 0.173 | 0.091 | 3 | 2,6,13 |
| J2325.2+3957 | 351.3245 | 39.9601 | BLLAC | 0.936 | - | 1 | 3 |
| J2325.4−3559 | 351.3692 | −35.9651 | AMB | 0.174 | - | 1 | 6 |
| J2325.4−4800 | 351.3620 | −48.0048 | BLLAC | 0.124 | 0.023 | 4 | 2,6,12a,13 |
| J2325.6+1644 | 351.4088 | 16.7785 | BLLAC | 0.356 | 0.269 | 2 | 3,13 |
| J2325.7+1821 | 351.4498 | 18.3699 | UNCL | 0.413 | 0.185 | 8 | 3,4,6,7,8,9,12b,13 |
| J2326.2+0113 | 351.6068 | 1.2024 | FSRQ | 0.648 | 0.291 | 4 | 1,2,3,13 |
| J2326.9−0201 | 351.7241 | −2.0372 | MIS | 0.161 | 0.014 | 8 | 5,6,7,8,9,11,12b,13 |
| J2327.4+0444 | 351.8906 | 4.7951 | UNCL | 0.254 | 0.061 | 8 | 3,4,6,7,8,9,12b,13 |
| J2327.5+0939 | 351.8899 | 9.6693 | FSRQ | 0.717 | 0.796 | 2 | 3,13 |
| J2328.3−4036 | 352.0803 | −40.5861 | FSRQ | 0.146 | - | 1 | 13 |
| J2329.0+0832 | 352.2741 | 8.5711 | FSRQ | 0.751 | 0.139 | 3 | 1,3,13 |
| J2329.2+3755 | 352.3094 | 37.9040 | BLLAC | 1.363 | - | 1 | 3 |
| J2329.3−4733 | 352.3238 | −47.5053 | FSRQ | 0.642 | 0.810 | 2 | 2,13 |
| J2329.3−4955 | 352.3370 | −49.9280 | FSRQ | 0.755 | - | 1 | 13 |
| J2329.7−2118 | 352.4234 | −21.2957 | MIS | 0.025 | 0.008 | 3 | 5,6,11 |
| J2330.3−2332 | 352.5674 | −23.6115 | UNCL | 1.191 | 1.189 | 2 | 3,4 |
| J2330.5+1102 | 352.6702 | 11.0052 | FSRQ | 1.178 | 0.399 | 3 | 1,3,13 |
| J2330.6−3726 | 352.6491 | −37.4105 | BLLAC | 0.195 | 0.001 | 2 | 5,6 |
| J2331.0−2147 | 352.7668 | −21.8042 | FSRQ | 1.139 | - | 1 | 3 |
| J2331.1−1653 | 352.7311 | −16.9443 | UNCL | 1.282 | 0.109 | 2 | 3,4 |
| J2331.3−1558 | 352.9111 | −15.9492 | FSRQ | 1.225 | - | 1 | 3 |
| J2331.5−0258 | 352.8040 | −3.0251 | UNCL | 0.560 | 0.266 | 4 | 1,3,4,13 |
| J2332.1−4118 | 353.0794 | −41.3104 | FSRQ | 0.344 | 0.275 | 2 | 2,13 |
| J2333.4−0133 | 353.3195 | −1.5187 | FSRQ | 0.923 | 0.399 | 4 | 1,2,3,13 |
| J2334.2+0736 | 353.5535 | 7.6077 | FSRQ | 0.899 | 1.071 | 2 | 3,13 |
| J2334.8+1432 | 353.7243 | 14.5374 | BLLAC | 0.877 | 0.570 | 3 | 1,3,13 |
| J2334.9−2346 | 353.4802 | −23.7280 | CLAGN | 0.041 | 0.017 | 4 | 3,5,6,11 |
| J2335.4−0128 | 353.8351 | −1.5193 | FSRQ | 0.682 | 0.495 | 4 | 1,2,3,13 |
| J2336.5−7622 | 354.1150 | −76.3439 | UNCL | 0.147 | - | 1 | 6 |
| J2336.6+2356 | 354.1754 | 23.9248 | MIS | 0.068 | 0.018 | 8 | 5,6,7,8,9,11,12b,13 |
| J2336.6−4115 | 354.1416 | −41.2561 | FSRQ | 0.715 | 0.153 | 2 | 2,13 |
| J2336.9−5859 | 354.3617 | −59.0205 | UNCL | 0.672 | 0.430 | 2 | 2,13 |
| J2338.0−0230 | 354.4889 | −2.5160 | FSRQ | 0.590 | 0.140 | 3 | 1,3,13 |
| J2338.1+0325 | 354.5319 | 3.4469 | CLAGN | 0.268 | 0.092 | 3 | 3,12b,13 |
| J2338.9+2124 | 354.7349 | 21.4115 | BLLAC | 0.650 | 0.693 | 2 | 3,13 |
| J2339.2−7403 | 354.8370 | −74.0766 | BLLAC | 0.139 | 0.021 | 2 | 5,6 |
| J2339.3−2656 | 354.8239 | −26.9442 | UNCL | 1.407 | - | 1 | 3 |
| J2339.6+0242 | 354.8738 | 2.7348 | FSRQ | 0.807 | 0.177 | 2 | 1,13 |
| J2340.5+3854 | 355.1786 | 38.9199 | UNCL | 0.293 | 0.143 | 2 | 4,6 |
| J2340.8+8015 | 355.2260 | 80.2544 | BLLAC | 0.157 | - | 1 | 6 |
| J2341.8−2917 | 355.3740 | −29.3208 | MIS | 0.029 | 0.008 | 3 | 5,6,11 |
| J2343.6+3438 | 355.8899 | 34.6642 | BLLAC | 0.238 | 0.082 | 4 | 6,7,8,9 |
| J2343.7−5624 | 355.8629 | −56.4400 | MIS | 0.628 | 0.439 | 3 | 2,6,13 |
| J2343.9+0546 | 355.9835 | 5.7841 | BLLAC | 0.131 | 0.011 | 2 | 9,13 |
| J2345.2−1555 | 356.3019 | −15.9188 | CLAGN | 1.712 | - | 1 | 3 |
| J2346.7+0705 | 356.6664 | 7.0852 | BLLAC | 0.077 | 0.012 | 4 | 5,6,9,13 |
| J2346.7+8008 | 356.6067 | 80.1320 | BLLAC | - | - | - | |
| J2348.0−1630 | 357.0109 | −16.5200 | FSRQ | 1.167 | - | 1 | 3 |
| J2348.1−4934 | 357.3556 | −49.5407 | UNCL | 0.185 | 0.027 | 5 | 2,6,12a,12b,13 |
| J2348.3−6049 | 357.1084 | −60.8222 | UNCL | 0.708 | 0.143 | 2 | 2,13 |
| J2349.2+4535 | 357.3376 | 45.5945 | BLLAC | 0.819 | 0.159 | 2 | 3,4 |
| J2349.4+0534 | 357.3377 | 5.5777 | CLAGN | 0.466 | 0.313 | 5 | 3,7,8,9,13 |
| J2350.6−3005 | 357.6429 | −30.1012 | BLLAC | 0.134 | 0.052 | 2 | 6,11 |
| J2350.9−1416 | 357.7963 | −14.2664 | BLLAC | 0.127 | 0.009 | 5 | 5,6,11,12b,13 |
| J2351.3−7559 | 357.8172 | −76.0043 | UNCL | 0.245 | 0.073 | 2 | 4,6 |
| J2352.0+1750 | 358.0243 | 17.8205 | BLLAC | 0.448 | 0.431 | 2 | 3,13 |
| J2352.9+3031 | 358.2279 | 30.5060 | FSRQ | 0.871 | 0.506 | 3 | 1,3,13 |
| J2353.1−4806 | 358.2963 | −48.1012 | UNCL | 0.250 | 0.070 | 3 | 2,4,13 |
| J2353.5−1457 | 358.3379 | −14.9825 | UNCL | 0.624 | 0.165 | 2 | 3,4 |
| J2353.7−3037 | 358.4477 | −30.6301 | BLLAC | - | - | - | |
| J2353.8−3911 | 358.4292 | −39.2456 | UNCL | 0.447 | 0.097 | 3 | 2,12a,13 |
| J2354.1+2720 | 358.5092 | 27.3910 | UNCL | 0.722 | 0.293 | 3 | 1,3,13 |
| J2354.1−0958 | 358.5231 | −9.9636 | AMB | 1.003 | 0.116 | 2 | 1,13 |
| J2354.6+4554 | 358.5903 | 45.8845 | FSRQ | 0.833 | 0.599 | 2 | 3,6 |
| J2354.9+8151 | 359.0950 | 81.8812 | FSRQ | - | - | - | |
| J2355.7−3351 | 358.9110 | −33.8741 | UNCL | 0.900 | - | 1 | 4 |
| J2356.2+4036 | 359.0531 | 40.6131 | BLLAC | 0.094 | 0.005 | 3 | 5,6,11 |
| J2357.0−4840 | 359.3376 | −48.6384 | UNCL | 0.554 | 0.139 | 2 | 2,13 |
| J2357.4−0152 | 359.3547 | −1.8710 | BLLAC | 0.469 | 0.322 | 4 | 1,2,3,13 |
| J2357.4−1718 | 359.3749 | −17.3009 | BLLAC | 2.331 | - | 1 | 3 |
| J2357.8−5311 | 359.4719 | −53.1871 | FSRQ | 0.551 | 0.201 | 2 | 2,13 |
| J2358.0−4601 | 359.5089 | −45.9219 | FSRQ | 0.488 | 0.318 | 2 | 2,13 |
| J2358.1−2853 | 359.5707 | −28.8928 | UNCL | 0.891 | 0.256 | 2 | 3,4 |
| J2358.3+3830 | 359.6049 | 38.4824 | SEY | 0.186 | 0.019 | 2 | 4,6 |
| J2358.3−1021 | 359.5453 | −10.3357 | FSRQ | 0.967 | 0.624 | 3 | 1,3,13 |
| J2358.5−1808 | 359.6535 | −18.1215 | BLLAC | 1.174 | - | 1 | 3 |
| J2359.0+3922 | 359.7494 | 39.3745 | FSRQ | 1.131 | - | 1 | 3 |
| J2359.0−3038 | 359.7829 | −30.6280 | BLLAC | 0.133 | - | 1 | 6 |
| J2359.3+0215 | 359.8210 | 2.2556 | BLLAC | 0.877 | 0.461 | 5 | 1,2,3,6,13 |
| J2359.3−2049 | 359.8314 | −20.7989 | BLLAC | 0.093 | 0.024 | 3 | 5,6,11 |
| J2359.9−3736 | 0.0351 | −37.6391 | UNCL | 0.257 | 0.004 | 4 | 6,12a,12b,13 |
| 1 | The original sample from 4FGL-DR2 consisted of 2982 point sources [18], but we updated it to 2980 when the DR3 was released, because J has no longer a counterpart and J is now associated with a millisecond pulsar. We did not include new sources added in the DR3. Hereinafter reference is always made to DR2, unless otherwise specified. |
| 2 | http://simbad.u-strasbg.fr/simbad/ (accessed on 30 August 2022). |
| 3 | http://ned.ipac.caltech.edu/ (accessed on 30 August 2022). |
| 4 | https://ui.adsabs.harvard.edu/ (accessed on 30 August 2022). |
| 5 | http://skyserver.sdss.org/DR16/en/home.aspx (accessed on 30 August 2022). |
| 6 | http://dr6.lamost.org/v2/ (accessed on 30 August 2022). |
| 7 | Although NED considers 1RXS J as the X-ray counterpart of NGC 7059, but, as we have shown, this is not the case. |
| 8 | The reclassification of the present sample of 2980 sources on a case-by-case basis required more than three years of one person’s almost full time. |
| 9 | https://iopscience.iop.org/article/10.1088/0004-637X/748/1/49 (accessed on 30 August 2022). |
| 10 | http://skyserver.sdss.org/DR16//en/tools/explore/summary.aspx?ra=220.9871&dec=25.029 (accessed on 30 August 2022). |
| 11 | http://skyserver.sdss.org/DR16//en/tools/explore/summary.aspx?ra=0.384875&dec=21.226739 (accessed on 30 August 2022). |
| 12 | https://www.cosmos.esa.int/web/life-cycle-of-agn/home (accessed on 30 August 2022). |
| 13 | http://skyserver.sdss.org/DR16//en/tools/explore/summary.aspx?ra=200.2967&dec=22.27 (accessed on 30 August 2022). |
| 14 | See here https://fermi.gsfc.nasa.gov/science/instruments/table1-1.html (accessed on 30 August 2022) for a comparison between EGRET and LAT instruments. |
| 15 | http://skyserver.sdss.org/DR16//en/tools/chart/navi.aspx?ra=243.921721316305&dec=47.1866096751966&scale=0.2 (accessed on 30 August 2022). |
References
- Rees, M.J. Appearance of Relativistically Expanding Radio Sources. Nature 1966, 211, 468–470. [Google Scholar] [CrossRef]
- Schmidt, M. Space Distribution and Luminosity Functions of Quasi-Stellar Radio Sources. Astrophys. J. 1968, 151, 393–409. [Google Scholar] [CrossRef]
- Fanaroff, B.L.; Riley, J.M. The morphology of extragalactic radio sources of high and low luminosity. Mon. Not. R. Astron. Soc. 1974, 167, 31P–35P. [Google Scholar] [CrossRef] [Green Version]
- Blandford, R.D.; Rees, M.J. Some comments on radiation mechanisms in Lacertids. In Pittsburgh Conference on BL Lac Objects; Wolfe, A.M., Ed.; University of Pittsburgh: Pittsburgh, PA, USA, 1978; pp. 328–347. [Google Scholar]
- Orr, M.J.L.; Browne, I.W.A. Relativistic beaming and quasar statistics. Mon. Not. R. Astron. Soc. 1982, 200, 1067–1080. [Google Scholar] [CrossRef]
- Barthel, P.D. Is every quasar beamed? Astrophys. J. 1989, 336, 606–611. [Google Scholar] [CrossRef]
- Urry, C.M.; Padovani, P. Unified Schemes for Radio-Loud Active Galactic Nuclei. Publ. Astron. Soc. Pac. 1995, 107, 803–845. [Google Scholar] [CrossRef] [Green Version]
- Ghisellini, G.; Celotti, A.; Fossati, G.; Maraschi, L.; Comastri, A. A theoretical unifying scheme for gamma-ray bright blazars. Mon. Not. R. Astron. Soc. 1998, 301, 451–468. [Google Scholar] [CrossRef] [Green Version]
- Padovani, P. On the two main classes of active galactic nuclei. Nat. Astron. 2017, 1, 0194. [Google Scholar] [CrossRef] [Green Version]
- Blandford, R.; Meier, D.; Readhead, A. Relativistic Jets from Active Galactic Nuclei. Annu. Rev. Astron. Astrophys. 2019, 57, 467–509. [Google Scholar] [CrossRef] [Green Version]
- Komossa, S. Multi-wavelength properties of radio-loud Narrow-line Seyfert 1 galaxies. Proc. Sci. 2018, 328, 15. [Google Scholar]
- Foschini, L. Jetted Narrow-Line Seyfert 1 Galaxies & Co.: Where Do We Stand? Universe 2020, 6, 136. [Google Scholar]
- Berton, M.; Caccianiga, A.; Foschini, L.; Peterson, B.; Mathur, S.; Terreran, G.; Ciroi, S.; Congiu, E.; Cracco, V.; Frezzato, M.; et al. Compact steep-spectrum sources as the parent population of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies. Astron. Astrophys. 2016, 591, A98. [Google Scholar] [CrossRef]
- Foschini, L. What we talk about when we talk about blazars? Front. Astron. Space Sci. 2017, 4, 6. [Google Scholar] [CrossRef] [Green Version]
- Romano, P.; Vercellone, S.; Foschini, L.; Tavecchio, F.; Landoni, M.; Knödlseder, J. Prospects for gamma-ray observations of narrow-line Seyfert 1 galaxies with the Cherenkov Telescope Array. Mon. Not. R. Astron. Soc. 2018, 481, 5046–5061. [Google Scholar] [CrossRef] [Green Version]
- Abdollahi, S. et al. [Fermi LAT Collaboration] Fermi Large Area Telescope Fourth Source Catalog. Astrophys. J. Suppl. Ser. 2020, 247, 33. [Google Scholar] [CrossRef] [Green Version]
- Ajello, M. et al. [Fermi LAT Collaboration] The Fourth Catalog of Active Galactic Nuclei detected by the Fermi Large Area Telescope. Astrophys. J. 2020, 892, 105. [Google Scholar] [CrossRef]
- Foschini, L.; Lister, M.L.; Antón, S.; Berton, M.; Ciroi, S.; Marchã, M.J.M.; Tornikoski, M.; Järvelä, E.; Romano, P.; Vercellone, S.; et al. A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei—Preliminary Results. Universe 2021, 7, 372. [Google Scholar] [CrossRef]
- Ghisellini, G.; Tavecchio, F.; Foschini, L.; Bonnoli, G.; Tagliaferri, G. The red blazar PMN J2345-1555 becomes blue. Mon. Not. R. Astron. Soc. Lett. 2013, 432, L66–L70. [Google Scholar] [CrossRef] [Green Version]
- Hernández-García, L.; Panessa, F.; Giroletti, M.; Ghisellini, G.; Bassani, L.; Masetti, N.; Pović, M.; Bazzano, A.; Ubertini, P.; Malizia, A.; et al. Restarting activity in the nucleus of PBC J2333.9-2343. An extreme case of jet realignment. Astron. Astrophys. 2017, 603, A131. [Google Scholar] [CrossRef] [Green Version]
- Kaur, A.; Falcone, A.D.; Stroh, M.D.; Kennea, J.A.; Ferrara, E.C. Classification of New X-Ray Counterparts for Fermi Unassociated Gamma-Ray Sources Using the Swift X-Ray Telescope. Astrophys. J. 2019, 887, 18. [Google Scholar] [CrossRef] [Green Version]
- Kerby, S.; Kaur, A.; Falcone, A.D.; Stroh, M.C.; Ferrara, E.C.; Kennea, J.A.; Colosimo, J. X-Ray Spectra and Multiwavelength Machine Learning Classification for Likely Counterparts to Fermi 3FGL Unassociated Sources. Astron. J. 2021, 161, 154. [Google Scholar] [CrossRef]
- Norris, R.P.; Marvil, J.; Collier, J.D.; Kapińska, A.D.; O’Brien, A.N.; Rudnick, L.; Andernach, H.; Asorey, J.; Brown, M.J.I.; Brüggen, M.; et al. The Evolutionary Map of the Universe pilot survey. Publ. Astron. Soc. Australia 2021, 38, e046. [Google Scholar] [CrossRef]
- Shaw, M.S.; Romani, R.W.; Cotter, G.; Healey, S.E.; Michelson, P.F.; Readhead, A.C.S.; Richards, J.L.; Max-Moerbeck, W.; King, O.G.; Potter, W.J. Spectroscopy of Broad-line Blazars from 1LAC. Astrophys. J. 2012, 748, 49. [Google Scholar] [CrossRef]
- Rakshit, S.; Stalin, C.S.; Kotilainen, J. Spectral Properties of Quasars from Sloan Digital Sky Survey Data Release 14: The Catalog. Astrophys. J. Suppl. Ser. 2020, 249, 17. [Google Scholar] [CrossRef]
- Ahnen, M.L.; Ansoldi, S.; Antonelli, L.A.; Antoranz, P.; Babic, A.; Banerjee, B.; Bangale, P.; Barres de Almeida, U.; Barrio, J.A.; Bednarek, W.; et al. (MAGIC Coll.) Very High Energy γ-Rays from the Universe’s Middle Age: Detection of the z=0.940 Blazar PKS 1441+25 with MAGIC. Astrophys. J. Lett. 2015, 815, L23. [Google Scholar] [CrossRef] [Green Version]
- Chen, K.; Halpern, J.P. Structure of Line-emitting Accretion Disks in Active Galactic Nuclei: ARP 102B. Astrophys. J. 1989, 344, 115–124. [Google Scholar] [CrossRef]
- Shen, Y.; Ho, L.C. The diversity of quasars unified by accretion and orientation. Nature 2014, 513, 210–213. [Google Scholar] [CrossRef] [Green Version]
- Panda, S.; Marziani, P.; Czerny, B. The Quasar Main Sequence Explained by the Combination of Eddington Ratio, Metallicity, and Orientation. Astrophys. J. 2019, 882, 79. [Google Scholar] [CrossRef] [Green Version]
- Marziani, P.; Bon, E.; Bon, N.; D’Onofrio, M.; Punsly, B.; Śniegowska, M.; Czerny, B.; Panda, S.; Martnez Aldama, M.L.; del Olmo, A.; et al. The main sequence of quasars: The taming of the extremes. Astron. Nachr. 2022, 343, e210082. [Google Scholar] [CrossRef]
- Marziani, P.; Sulentic, J.W.; Plauchu-Frayn, I.; del Olmo, A. Low-ionization Outflows in High Eddington Ratio Quasars. Astrophys. J. 2013, 764, 150. [Google Scholar] [CrossRef] [Green Version]
- Punsly, B.; Marziani, P.; Berton, M.; Kharb, P. The Extreme Red Excess in Blazar Ultraviolet Broad Emission Lines. Astrophys. J. 2020, 903, 44. [Google Scholar] [CrossRef]
- Ho, L.C.; Kim, M. The Black Hole Mass Scale of Classical and Pseudo Bulges in Active Galaxies. Astrophys. J. 2014, 789, 17. [Google Scholar] [CrossRef]
- Berton, M.; Foschini, L.; Ciroi, S.; Cracco, V.; La Mura, G.; Lister, M.L.; Mathur, S.; Peterson, B.M.; Richards, J.L.; Rafanelli, P. Parent population of flat-spectrum radio-loud narrow-line Seyfert 1 galaxies. Astron. Astrophys. 2015, 578, A28. [Google Scholar] [CrossRef] [Green Version]
- Heinz, S.; Sunyaev, R.A. The non-linear dependence of flux on black hole mass and accretion rate in core-dominated jets. Mon. Not. R. Astron. Soc. 2003, 343, L59–L64. [Google Scholar] [CrossRef] [Green Version]
- Abdo, A.A. et al. [Fermi LAT Collaboration] Fermi/Large Area Telescope discovery of gamma-ray emission from a relativistic jet in the narrow-line quasar PMN J0948+0022. Astrophys. J. 2009, 699, 976–984. [Google Scholar] [CrossRef] [Green Version]
- Foschini, L.; Ghisellini, G.; Kovalev, Y.Y.; Lister, M.L.; D’Ammando, F.; Thompson, D.J.; Tramacere, A.; Angelakis, E.; Donato, D.; Falcone, A.; et al. The first gamma-ray outburst of a narrow-line Seyfert 1 galaxy: The case of PMN J0948+0022 in 2010 July. Mon. Not. R. Astron. Soc. 2011, 413, 1671–1677. [Google Scholar] [CrossRef] [Green Version]
- Paliya, V.S.; Sahayanathan, S.; Parker, M.L.; Fabian, A.C.; Stalin, C.S.; Anjum, A.; Pandey, S.B. The Peculiar Radio-loud Narrow Line Seyfert 1 Galaxy 1H 0323+342. Astrophys. J. 2014, 789, 143. [Google Scholar] [CrossRef] [Green Version]
- Paliya, V.S.; Stalin, C.S. The First GeV Outburst of the Radio-loud Narrow-line Seyfert 1 Galaxy PKS 1502+036. Astrophys. J. 2016, 820, 52. [Google Scholar] [CrossRef] [Green Version]
- Hartman, R.C.; Bertsch, D.L.; Bloom, S.D.; Chen, A.W.; Deines-Jones, P.; Esposito, J.A.; Fichtel, C.E.; Friedlander, D.P.; Hunter, S.D.; McDonald, L.M.; et al. The Third EGRET Catalog of High-Energy Gamma-Ray Sources. Astrophys. J. Suppl. Ser. 1999, 123, 79–202. [Google Scholar] [CrossRef] [Green Version]
- Wu, Q.; Shen, Y. A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16. arXiv 2022, arXiv:2209.03987. [Google Scholar]
- Nandikotkur, G.; Jahoda, K.M.; Hartman, R.C.; Mukherjee, R.; Sreekumar, P.; Böttcher, M.; Sambruna, R.M.; Swank, J.H. Does the Blazar Gamma-Ray Spectrum Harden with Increasing Flux? Analysis of 9 Years of EGRET Data. Astrophys. J. 2007, 657, 706–724. [Google Scholar] [CrossRef] [Green Version]
- Readhead, A.C.S.; Ravi, V.; Liodakis, I.; Lister, M.L.; Singh, V.; Aller, M.F.; Blandford, R.D.; Browne, I.W.A.; Gorjian, V.; Grainge, K.J.B.; et al. The Relativistic Jet Orientation and Host Galaxy of the Peculiar Blazar PKS 1413+135. Astrophys. J. 2021, 907, 61. [Google Scholar] [CrossRef]
- Hakobyan, A.A.; Adibekyan, V.Z.; Aramyan, L.S.; Petrosian, A.R.; Gomes, J.M.; Mamon, G.A.; Kunth, D.; Turatto, M. Supernovae and their host galaxies. I. The SDSS DR8 database and statistics. Astron. Astrophys. 2012, 544, A81. [Google Scholar] [CrossRef]
- Heidt, J.; Nilsson, K.; Fried, J.W.; Takalo, L.O.; Sillanpää, A. 1ES 1741+196: A BL Lacertae object in a triplet of interacting galaxies? Astron. Astrophys. 1999, 348, 113–116. [Google Scholar]
- Véron-Cetty, M.-P.; Véron, P. Spectroscopic observatioons of sixteen BL Lacertae candidates. Astron. Astrophys. Suppl. Ser. 1993, 100, 521–529. [Google Scholar]
- Hunstead, R.W.; Murdoch, H.S.; Condon, J.J.; Phillips, M.M. A QSO with precessing jets: 2300-189. Mon. Not. R. Astron. Soc. 1984, 207, 55–71. [Google Scholar] [CrossRef]
Figure 1.
Distribution of the present list of gamma-ray sources in the sky (Galactic coordinates, Aitoff projection) according to the new classification.
Figure 1.
Distribution of the present list of gamma-ray sources in the sky (Galactic coordinates, Aitoff projection) according to the new classification.
Figure 2.
Distribution of the redshifts (spectroscopic and photometric).
Figure 3.
Comparison of photometric redshift with spectroscopic one, for those sources having both values. The blue line shows the function .
Figure 3.
Comparison of photometric redshift with spectroscopic one, for those sources having both values. The blue line shows the function .
Figure 4.
Distribution of the difference between the photometric and spectroscopic redshifts.
Figure 5.
Reanalysis of SDSS spectrum of PKS : (left panel) H and [OIII] complex; (right panel) MgII. Both H and MgII display a clear red wing, and were fitted with a narrower component plus a broader red one (blue dashed lines). The SDSS spectrum is represented by a black continuous line, while the individual components are depicted with dashed blue lines. The model sum of the different components is a red continuous line.
Figure 5.
Reanalysis of SDSS spectrum of PKS : (left panel) H and [OIII] complex; (right panel) MgII. Both H and MgII display a clear red wing, and were fitted with a narrower component plus a broader red one (blue dashed lines). The SDSS spectrum is represented by a black continuous line, while the individual components are depicted with dashed blue lines. The model sum of the different components is a red continuous line.
Table 1.
Distribution of gamma-ray emitting jetted AGN according to the present work and comparison with the original 4FGL subsample. Columns: (1) Classification according to our criteria; (2) number N of sources of the corresponding class; (3) percentage of sources with spectroscopic redshift z; (4) number of sources with the same (or similar) classification in the 4FGL. The notes at the end of the table explain the differences between the present classification criteria and those of the 4FGL.
Table 1.
Distribution of gamma-ray emitting jetted AGN according to the present work and comparison with the original 4FGL subsample. Columns: (1) Classification according to our criteria; (2) number N of sources of the corresponding class; (3) percentage of sources with spectroscopic redshift z; (4) number of sources with the same (or similar) classification in the 4FGL. The notes at the end of the table explain the differences between the present classification criteria and those of the 4FGL.
| Classification | N | z | 4FGL |
|---|---|---|---|
| BL Lac Object (BLLAC) | 1207 | 47.2% | 1204 |
| Flat-spectrum radio quasar (FSRQ) | 695 | 99.7% | 703 |
| Misaligned AGN (MIS ) | 85 | 96.5% | 45 |
| Narrow-Line Seyfert 1 galaxy (NLS1) | 24 | 100% | 9 |
| Seyfert galaxy (SEY ) | 32 | 100% | 0 |
| Ambiguous (AMB) | 42 | 69% | - |
| Changing-look AGN (CLAGN) | 34 | 100% | - |
| Unclassified (UNCL ) | 861 | 0.1% | 1009 |
| Total | 2980 | 49% | 2980 |
The MIS class includes the 4FGL classes RDG/rdg, SSRQ/ssrq, and CSS/css. Seyfert class includes Seyfert 1, 2, intermediate, and LINERS. The UNCL class includes the 4FGL classes BCU/bcu, and UNK/unk. Photometric redshift is also available for another 43% of sources. Therefore, 93% of sources do have a redshift value. 4FGL contains also 10 sources classified as non-blazar active galaxy (AGN/agn), which were reclassified as BLLAC (1), MIS (3), CLAGN (3), UNCL (3).
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Foschini, L.; Lister, M.L.; Andernach, H.; Ciroi, S.; Marziani, P.; Antón, S.; Berton, M.; Dalla Bontà, E.; Järvelä, E.; Marchã, M.J.M.; et al. A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei. Universe 2022, 8, 587. https://doi.org/10.3390/universe8110587
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Foschini L, Lister ML, Andernach H, Ciroi S, Marziani P, Antón S, Berton M, Dalla Bontà E, Järvelä E, Marchã MJM, et al. A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei. Universe. 2022; 8(11):587. https://doi.org/10.3390/universe8110587
Chicago/Turabian StyleFoschini, Luigi, Matthew L. Lister, Heinz Andernach, Stefano Ciroi, Paola Marziani, Sonia Antón, Marco Berton, Elena Dalla Bontà, Emilia Järvelä, Maria J. M. Marchã, and et al. 2022. "A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei" Universe 8, no. 11: 587. https://doi.org/10.3390/universe8110587
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