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The XMM-SERVS survey: New XMM-Newton point-source catalogue for the XMM-LSS field

  • C. T.J. Chen
  • , W. N. Brandt
  • , B. Luo
  • , P. Ranalli
  • , G. Yang
  • , D. M. Alexander
  • , F. E. Bauer
  • , D. D. Kelson
  • , M. Lacy
  • , K. Nyland
  • , P. Tozzi
  • , F. Vito
  • , M. Cirasuolo
  • , R. Gilli
  • , M. J. Jarvis
  • , B. D. Lehmer
  • , M. Paolillo
  • , D. P. Schneider
  • , O. Shemmer
  • , I. Smail
  • M. Sun, M. Tanaka, M. Vaccari, C. Vignali, Y. Q. Xue, M. Banerji, K. E. Chow, B. Häußler, R. P. Norris, J. D. Silverman, J. R. Trump

Research output: Contribution to journalArticlepeer-review

Abstract

We present an X-ray point-source catalogue from the XMM-Large Scale Structure (XMMLSS) survey region, one of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields. We target the XMM-LSS region with 1.3 Ms of new XMM-Newton AO-15 observations, transforming the archival X-ray coverage in this region into a 5.3 deg2 contiguous field with uniform X-ray coverage totaling 2.7 Ms of flare-filtered exposure, with a 46 ks median PN exposure time. We provide an X-ray catalogue of 5242 sources detected in the soft (0.5-2 keV), hard (2-10 keV), and/or full (0.5-10 keV) bands with a 1 per cent expected spurious fraction determined from simulations. A total of 2381 new X-ray sources are detected compared to previous source catalogues in the same area. Our survey has flux limits of 1.7 × 10-15, 1.3 × 10-14, and 6.5 × 10-15 erg cm-2 s-1 over 90 per cent of its area in the soft, hard, and full bands, respectively, which is comparable to those of the XMM-COSMOS survey. We identify multiwavelength counterpart candidates for 99.9 per cent of the X-ray sources, of which 93 per cent are considered as reliable based on their matching likelihood ratios. The reliabilities of these high-likelihood-ratio counterparts are further confirmed to be ≈97 per cent reliable based on deep Chandra coverage over ≈5 per cent of the XMM-LSS region. Results of multiwavelength identifications are also included in the source catalogue, along with basic optical-to-infrared photometry and spectroscopic redshifts from publicly available surveys. We compute photometric redshifts for X-ray sources in 4.5 deg2 of our field where forced-aperture multiband photometry is available; > 70 per cent of the X-ray sources in this subfield have either spectroscopic or high-quality photometric redshifts.

Original languageEnglish (US)
Pages (from-to)2132-2163
Number of pages32
JournalMonthly Notices of the Royal Astronomical Society
Volume478
Issue number2
DOIs
StatePublished - Aug 1 2018

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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