The Remarkable X-ray Spectra and Variability of the Ultraluminous Weak-Line Quasar SDSS J1521+5202
Shouyi Wang, W. Niel Brandt, Bin Luo, Zhibo Yu, Fan Zou, Qingling Ni,, Fabio Vito

TL;DR
This study investigates the extreme X-ray variability of the ultraluminous weak-line quasar SDSS J1521+5202, revealing insights into its spectral properties and supporting a model involving a thick disk and outflow causing variable absorption.
Contribution
It provides the first detailed X-ray spectral and variability analysis of SDSS J1521+5202, supporting the thick-disk plus outflow model for WLQs with new observational evidence.
Findings
X-ray flux varies by up to a factor of 32 over 17 years.
2023 spectrum shows power-law with intrinsic absorption, consistent with typical WLQ emission.
2013 spectrum indicates spectral complexity not explained by simple models.
Abstract
We present a focused X-ray and multiwavelength study of the ultraluminous weak-line quasar (WLQ) SDSS J1521+5202, one of the few X-ray weak WLQs that is amenable to basic X-ray spectral and variability investigations. J1521+5202 shows striking X-ray variability during 2006--2023, by up to a factor of in 0.5--2 keV flux, and our new 2023 Chandra observation caught it in its brightest X-ray flux state to date. Concurrent infrared/optical observations show only mild variability. The 2023 Chandra spectrum can be acceptably described by a power law with intrinsic X-ray absorption, and it reveals a nominal intrinsic level of X-ray emission relative to its optical/ultraviolet emission. In contrast, an earlier Chandra spectrum from 2013 shows apparent spectral complexity that is not well fit by a variety of models, including ionized-absorption or standard Compton-reflection models.…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Galaxies: Formation, Evolution, Phenomena · Astrophysics and Cosmic Phenomena
