University of Hertfordshire

From the same journal

From the same journal

A Multi-Mission Catalogue of Ultraluminous X-ray Source Candidates

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Documents

  • D. J. Walton
  • A. D. A. Mackenzie
  • H. Gully
  • N. R. Patel
  • T. P. Roberts
  • H. P. Earnshaw
  • S. Mateos
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Original languageEnglish
Pages (from-to)1587–1604
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume509
Issue2
Early online date20 Oct 2021
DOIs
Publication statusPublished - 1 Jan 2022

Abstract

We present a new, multi-mission catalogue of ultraluminous X-ray source (ULX) candidates, based on recent data releases from each of the XMM-Newton, Swift and Chandra observatories (the 4XMM-DR10, 2SXPS and CSC2 catalogues, respectively). This has been compiled by cross-correlating each of these X-ray archives with a large sample of galaxies primarily drawn from the HyperLEDA archive. Significant efforts have been made to clean the sample of known non-ULX contaminants (e.g. foreground stars, background AGN, supernovae), and also to identify ULX candidates that are common to the different X-ray catalogues utilized, allowing us to produce a combined 'master' list of unique sources. Our sample contains 1843 ULX candidates associated with 951 different host galaxies, making it the largest ULX catalogue compiled to date. Of these, 689 sources are catalogued as ULX candidates for the first time. Our primary motivation is to identify new sources of interest for detailed follow-up studies, and within our catalogue we have already found one new extreme ULX candidate that has high S/N data in the archive: NGC 3044 ULX1. This source has a peak luminosity of $L_{\rm{X,peak}} \sim 10^{40}$ erg s$^{-1}$, and the XMM-Newton spectrum of the source while at this peak flux is very similar to other, better-studied extreme ULXs that are now understood to be local examples of super-Eddington accretion. This likely indicates that NGC 3044 ULX1 is another source accreting at super-Eddington rates. We expect that this catalogue will be a valuable resource for planning future observations of ULXs - both with our current and future X-ray facilities - to further improve our understanding of this enigmatic population.

Notes

© 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article has been accepted for publication in the Monthly Notices of the Royal Astronomical Society, which has been published in final form at https://doi.org/10.1093/mnras/stab3001.

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