X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
arXiv:2303.03438 · doi:10.3847/1538-4357/acc17e
Abstract
We investigate the extreme X-ray variability of a z = 1.608 active galactic nucleus in the 7 Ms Chandra Deep Field-South (XID 403), which showed two significant X-ray brightening events. In the first event, XID 403 brightened by a factor of in rest-frame days in the observed-frame 0.5-5 keV band. The event lasted for days, and then XID 403 dimmed by a factor of in days. After years in the rest frame (including long observational gaps), it brightened again with the 0.5-5 keV flux increasing by a factor of . The second event lasted over 251 days and the source remained bright until the end of the 7 Ms exposure. The spectrum is a steep power law (photon index ) without obscuration during the second outburst, and the rest-frame 2-10 keV luminosity reaches erg s; there is no significant spectral evolution within this epoch. The infrared-to-UV spectral energy distribution of XID 403 is dominated by the host galaxy. There is no significant optical/UV variability and -band (rest-frame $\unicode{xC5}$) brightening contemporaneous with the X-ray brightening. The extreme X-ray variability is likely due to two X-ray unveiling events, where the line of sight to the corona is no longer shielded by high-density gas clumps in a small-scale dust-free absorber. XID 403 is probably a high-redshift analog of local narrow-line Seyfert 1 galaxies, and the X-ray absorber is a powerful accretion-disk wind. On the other hand, we cannot exclude the possibility that XID 403 is an unusual candidate for tidal disruption events.
23 pages, 9 figures, accepted for publication in ApJ
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