Blazar Variability Across All Timescales

A special issue of Galaxies (ISSN 2075-4434).

Deadline for manuscript submissions: 30 July 2026 | Viewed by 1114

Special Issue Editors


E-Mail Website
Guest Editor
Department of Physics, Florida International University, Miami, FA 33199, USA
Interests: multi-frequency blazar variability; microvariability
Special Issues, Collections and Topics in MDPI journals

E-Mail Website
Guest Editor
Institute of Astronomy, The University of Zielona Gora, Zielona Gora, Poland
Interests: blazars multifrequency variability
Special Issues, Collections and Topics in MDPI journals

Special Issue Information

Dear Colleagues,

This Special Issue of Galaxies is intended to bring together papers on recent advances in understanding the physics of blazars through multifrequency variability. Papers covering frequency ranges from radio through gamma rays and timescales from microvariability to long-term variability (years) are encouraged. Observations and theories of line variability as well as continuum variability are encouraged. The physics behind these observations link the basic components of current AGN models: disk processes, jet processes, and broad line region processes. Bringing all of these together in a Special Issue highlights the current state of knowledge of these intriguing physics laboratories.

References:
Multifrequency Photo-polarimetric WEBT Observation Campaign on the Blazar S5 0716+714: Source Microvariability and Search for Characteristic Timescales, Bhatta, Webb et al. Ap J, 831, 2016.

Multi-frequency Blazar Micro-Variability as a Tool to Investigate Relativistic Jets, Webb, J. Galaxies, 4, 2016.

The 72-h WEBT Microvariability observation of blazar S5 0716 + 714 in 2009. Bhatta, G., Webb, J., et al. 2013, A&A 558, 92.

Microvariability and Long-Term Variability of Four Blazars. Howard, E., Webb, J. et al., 2004, AJ, 127, 1.

Multiband optical-NIR variability of blazars on diverse time-scales. Agarwal, A, Gupta, et al. MNRAS, 451, 3882.
Statistical Analysis of Microvariability Properties of the Blazar S5 0716+714 ApJ, 884, 92,2019, Xu, J, Hu, S., Webb, J.R., Bhatta, G., Jiang, Y, Chen, Xu, Alexeeva, S.,Li, Y. 
30 Years of Multifrequency Quasar Variability: A Personal Journey, Webb, J.R., Galaxies 9040069, 2021.
The Nature of Micro-Variability in Blazars, Webb, Arroyave, Laurence, Revesz, Bhatta, Hollingsworth., Dhalla, Howard and Cioffi.Galaxies, 9040114, 2021.
 The Structure of Micro-Variability in the WEBT BL Lacertae Observation, Webb, James R.; Sanz, Ivan Parra Galaxies, 11, 2023.
A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour Raiteri, C. M.; Villata, M.; Carnerero, M. I. and 96 more, 2024A&A...692A..48R2024/12.

Prof. Dr. James R. Webb
Dr. Gopal Bhatta
Guest Editors

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 250 words) can be sent to the Editorial Office for assessment.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Galaxies is an international peer-reviewed open access semimonthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 1500 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • blazars
  • blazar variability
  • multiwavelength variability of blazars
  • blazar jets
  • blazar line variability

Benefits of Publishing in a Special Issue

  • Ease of navigation: Grouping papers by topic helps scholars navigate broad scope journals more efficiently.
  • Greater discoverability: Special Issues support the reach and impact of scientific research. Articles in Special Issues are more discoverable and cited more frequently.
  • Expansion of research network: Special Issues facilitate connections among authors, fostering scientific collaborations.
  • External promotion: Articles in Special Issues are often promoted through the journal's social media, increasing their visibility.
  • Reprint: MDPI Books provides the opportunity to republish successful Special Issues in book format, both online and in print.

Further information on MDPI's Special Issue policies can be found here.

Published Papers (1 paper)

Order results
Result details
Select all
Export citation of selected articles as:

Research

22 pages, 4929 KB  
Article
Turbulent Cell Interpretation of Micro-Variability of BL Lacertae: Polarization
by James R. Webb, Claudia Garcia, Jade Irizarry, Dennis Moreno and Alan P. Marscher
Galaxies 2026, 14(2), 24; https://doi.org/10.3390/galaxies14020024 - 17 Mar 2026
Viewed by 614
Abstract
We present the results of the analysis of nine polarization and micro-variability observations of BL Lacertae using a turbulent cell model. We perform a similar analysis of a simulated TEMZ light curve generated with the Turbulent Extreme Multi-Zone (TEMZ) model and compare the [...] Read more.
We present the results of the analysis of nine polarization and micro-variability observations of BL Lacertae using a turbulent cell model. We perform a similar analysis of a simulated TEMZ light curve generated with the Turbulent Extreme Multi-Zone (TEMZ) model and compare the results. Observations of short-timescale variability of flux and polarization are important to understanding the physical conditions in the blazar jet. We find that the micro-variations exhibited by the BL Lac data analyzed here are well fit by a turbulent cell model consisting of multiple pulses, with an average correlation coefficient of r~0.94. We compare these results with a similar analysis of light and polarization curves from a TEMZ simulation, which employs many more cells with physical properties related across cells following the Kolmogorov spectrum. We find that groups of turbulent cells identified in the TEMZ model by our analysis are similar to the input cell structure of the simulation. We find that the results from the actual BL Lac light curve and polarization curves match very well with the results from analyzing the TEMZ simulated light curves. We find no apparent trend or direct correlation between the cells determined from the flux curves and polarization degree, or polarization angle in either the BL Lac or the TEMZ data sets. Full article
(This article belongs to the Special Issue Blazar Variability Across All Timescales)
Show Figures

Figure A1

Back to TopTop