A reverberation mapping study of a highly variable AGN 6dFGS gJ022550.0-060145
arxiv(2024)
摘要
We use LCOGT observations (MJD 59434-59600) with a total exposure time of
≃ 50 hours and a median cadence of 0.5 days to measure the inter-band
time delays (with respect to u) in the g, r, and i continua of a highly
variable AGN, 6dFGS gJ022550.0-060145. We also calculate the expected time
delays of the X-ray reprocessing of a static Shakura & Sunyaev disk (SSD)
according to the sources' luminosity and virial black-hole mass; the two
parameters are measured from the optical spectrum of our spectroscopic
observation via the Lijiang 2.4 telescope. It is found that the
ratio of the measured time delays to the predicted ones is 2.6_-1.3^+1.3.
With optical light curves (MJD 53650-59880) from our new LCOGT and archival
ZTF, Pan-SATRRS, CSS, and ATLAS observations, and infrared (IR) WISE data (MJD
55214-59055), we also measured time delays between WISE W1/W2 and the
optical emission. W1 and W2 have time delays (with respect to V),
9.6^+2.9_-1.6× 10^2 days and 1.18^+0.13_-0.10× 10^3 days
in the rest-frame, respectively; hence, the dusty torus of 6dFGS
gJ022550.0-060145 should be compact. The time delays of W1 and W2 bands are
higher than the dusty torus size-luminosity relationship of . By
comparing the IR and optical variability amplitude, we find that the dust
covering factors of W1 and W2 emission regions are 0.7 and 0.6,
respectively. Future broad emission-line reverberation mapping of this target
and the results of this work enable us to determine the sizes of the AGN main
components simultaneously.
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