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Galaxies 2017, 5(1), 7; doi:10.3390/galaxies5010007

Optical and Gamma-Ray Variability of the vRL NLSy1 Galaxy, 1H 0323+342

Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30302-3965, USA
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Author to whom correspondence should be addressed.
Academic Editors: Jose L. Gómez, Alan P. Marscher and Svetlana G. Jorstad
Received: 2 September 2016 / Revised: 10 November 2016 / Accepted: 11 November 2016 / Published: 20 January 2017
(This article belongs to the Special Issue Blazars through Sharp Multi-wavelength Eyes)
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Abstract

1H 0323+342 was one of the first vRLNLSy1 galaxies detected at gamma-rays with the Fermi-LAT and is one of the brightest of this class observed at optical wavelengths. We report the results of monitoring the optical flux, polarization and the gamma-ray flux of 1H 0323+342 during the past ~5 years. In some cases, the optical flux has been monitored on timescales as short as ~minutes simultaneously with two telescopes, demonstrating, for the first time, the reality of microvariability events with durations as short as ~15 min for this object. View Full-Text
Keywords: blazar; narrow line seyfert 1 galaxy; gamma-ray source blazar; narrow line seyfert 1 galaxy; gamma-ray source
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This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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MDPI and ACS Style

Miller, H.R.; Turner, C.S.; Maune, J.D.; Eggen, J.R. Optical and Gamma-Ray Variability of the vRL NLSy1 Galaxy, 1H 0323+342. Galaxies 2017, 5, 7.

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