X-Ray Absorption By WHIM in the Sculptor Wall
David A. Buote (1), Luca Zappacosta (1,2), Taotao Fang (1), Philip J., Humphrey (1), Fabio Gastaldello (1,3), and Gianpiero Tagliaferri (4) ((1) UC, Irvine, (2) INAF-Trieste, (3) INAF-Milano, (4) INAF-Brera)

TL;DR
This study reports the first simultaneous analysis of XMM and Chandra X-ray data detecting the WHIM in the Sculptor Wall, providing robust evidence for the missing baryons in large-scale cosmic structures.
Contribution
It presents the first robust detection of non-local WHIM via X-ray absorption using simultaneous XMM and Chandra observations with known redshift.
Findings
Detection of O vii K-alpha line at 3-sigma significance
Column density consistent with cosmological simulations
First simultaneous X-ray analysis confirming WHIM presence
Abstract
We present XMM RGS and Chandra LETG observations of the blazar, H 2356-309, located behind the Sculptor Wall, a large-scale galaxy structure expected to harbor high-density Warm-Hot Intergalactic Medium (WHIM). Our simultaneous analysis of the RGS and LETG spectra yields a 3-sigma detection of the crucial redshifted O vii K-alpha line with a column density (>~ 10^{16} cm^{-2}) consistent with similar large-scale structures produced in cosmological simulations. This represents the first detection of non-local WHIM from X-ray absorption studies where XMM and Chandra data are analyzed simultaneously and the absorber redshift is already known, thus providing robust evidence for the expected repository of the "missing baryons".
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