http://arxiv.org/abs/2301.01944
We present a long-term and intraday variability study on optical multiwaveband ($U!BV!RI$) data from the blazar AO 0235+164 collected by various telescopes for $\sim$44 years (1975–2019). The blazar was found to be significantly variable over the years in all wavebands with a variation of about six magnitudes between its low and active states. The variations in the different wavebands are highly correlated without any time lag. We did not observe any significant trend in color variation with time, but we observed a bluer-when-brighter trend between the $B-I$ color index and the $R$-magnitude. Optical $BV!R$-band spectral energy distributions always show a convex shape. Significant intraday variability was frequently seen in the quasi-simultaneous observations of AO\,0235+164 made on 22 nights in $R$ and $V$-bands by the CASLEO and CAHA telescopes during 1999–2019. We also estimated the central supermassive black-hole mass of $7.9\times10^7 M_{\odot}$ by analyzing the broad Mg II emission line in AO 0235+164’s spectrum. We briefly explore the probable physical scenarios responsible for the observed variability.
A. Roy, A. Gupta, V. Chitnis, et. al.
Fri, 6 Jan 23
25/55
Comments: 27 pages, 10 figures. Accepted for publication in The Astrophysical Journal Supplement Series (ApJS)