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arXiv · 1211.3082

The Extreme Optical Variability of J0948+0022

Jeremy D. Maune·H. Richard Miller·Joesph R. Eggen
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Abstract

We report on observations of the optical variability of the radio-loud, narrow-line Seyfert 1 galaxy J0948+0022 on time scales ranging from minutes to years. Implications regarding recent suggestions that the object may constitute a prototype for an emerging class of blazar-like objects similar to FSRQs are discussed. The optical microvariability observed for J0948+0022 is found to be similar to that found for a typical LBL blazar. Based on observations of J0948+0022 in a flaring state and a significantly lower state, one can demonstrate that these rapid variations are most likely originating in the relativistic jet and not in the accretion disk

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Jeremy D. Maune, H. Richard Miller, Joesph R. Eggen. 2012-11-13. The Extreme Optical Variability of J0948+0022. https://doi.org/10.1088/0004-637x/762/2/124

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