X-ray Absorption and Reprocessing in the $z \sim 2.5$ Lensed Quasar 2MASS J1042+1641
D. J. Walton, M. T. Reynolds, D. Stern, M. Brightman, C. Lemon

TL;DR
This study presents broadband X-ray observations of a high-redshift lensed quasar, revealing complex absorption and reprocessing features, and explores models of the reprocessing material, with implications for identifying such quasars.
Contribution
It provides the first broadband X-ray spectrum of a $z \\sim 2.5$ lensed quasar and compares reprocessing models, enhancing understanding of AGN structure and aiding in candidate identification.
Findings
Detected strong Compton-thin X-ray absorption ($N_H \\sim 3-4 \\times 10^{23}$ cm$^{-2}$)
Reprocessing can occur in either a torus or accretion disk model, both fitting the data
Supports using combined X-ray and IR surveys to identify lensed quasars
Abstract
We present new broadband X-ray observations of the lensed quasar 2MASS J1042+1641, combining -, and to provide coverage of the X-ray spectrum over the 0.340 keV bandpass in the observed frame, corresponding to the 1140 keV band in the rest-frame of 2MASS J1042+1641. The X-ray data show clear evidence for strong (but still Compton-thin) X-ray absorption, cm, in addition to significant reprocessing by Compton-thick material that must lie away from our line-of-sight to the central X-ray source. We test two different interpretations for the latter: first that the reprocessing occurs in a classic AGN torus, as invoked in unification models, and second that the reprocessing occurs in the accretion disc. Both models can successfully reproduce the observed spectra, and both imply that the source…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysical Phenomena and Observations
