SIMBAD references

2025MNRAS.539.2088S - Mon. Not. R. Astron. Soc., 539, 2088-2109 (2025/May-3)

X-ray absorption lines in FUV-detected quasars: I. Sample and analysis of the XMM-Newton and Chandra data.

SPENCE D., BONAMENTE M., AHORANTA J., WIJERS N., TUOMINEN T. and DE PLAA J.

Abstract (from CDS):

This paper presents initial results of a systematic search for resonance X-ray absorption lines from H-like O VIII and $He$-like O VII caused by the intervening warm-hot intergalactic medium (WHIM). The search is based on far ultra-violet redshift priors from O VI and H I broad Lyman $\alpha$ lines that were previously detected by HST and FUSE in a sample of 51 sources with either XMM-Newton or Chandra data, for a total X-ray redshift path of $\Delta z=10.9$. Of the 1224 absorption-line systems with FUV priors that were analysed, 33 systems feature an absorption-line feature detected with $\ge 99$ % confidence at the same redshift of the FUV prior, some coincident with previously reported absorption line detections. The ultimate goal of this search is to test the hypothesis that X-ray absorbing WHIM gas is the repository of the missing baryons in the local universe. Further results and the cosmological implications of this analysis are presented in a companion paper.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): quasars: absorption lines - cosmology: observations - X-rays: general

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 89

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