Search for intra-day optical variability in Mrk 501
Hai-Cheng Feng, H. T. Liu, X. L. Fan, Yinghe Zhao, J. M. Bai, Fang, Wang, D. R. Xiong, and S. K. Li

TL;DR
This study reports optical intra-day variability in Mrk 501, including a flare with a 26.7-minute darkening timescale, and uses this to estimate an upper limit on the black hole mass consistent with previous measurements.
Contribution
First detection of optical intra-day variability in Mrk 501 with detailed flare analysis and black hole mass estimation based on variability timescales.
Findings
Detected a 26.7-minute darkening timescale during a flare.
Estimated black hole mass upper limit of ~10^9.2 solar masses.
Results are consistent with previous black hole mass measurements.
Abstract
We present our observations of the optical intra-day variability (IDV) in -ray BL Lac object Mrk 501. The observations were run with the 1.02 m and 2.4 m optical telescopes at Yunnan Observatories from 2005 April to 2012 May. The light curve at the band on 2010 May 15 passes both variability tests (the test and the ANOVA test). A flare within the light curve on 2010 May 15 has a magnitude change mag, \textbf{a darkening timescale of 26.7 minutes}, and an amplitude of IDV . A decline \textbf{described by 11 consecutive flux measurements} within the flare can be fitted linearly with a Pearson's correlation coefficient at the confidence level of . Under the assumptions that the IDV is tightly connected to the mass of the black hole, \textbf{and that the…
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