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. SmailM. Sun, M. Tanaka, M. Vaccari, C. Vignali, Y. Q. Xue, M. Banerji, K. E. Chow, B. Haussler, R. P. Norris, J. D. Silverman, J. R. Trump

Research output: Contribution to journalArticlepeer-review

83 Citations (Scopus)

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 deg(2) 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 x 10(-15), 1.3 x 10(-14),and 6.5 x 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 approximate to 97 per cent reliable based on deep Chandra coverage over approximate to ≈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
Pages (from-to)2132-2163
Number of pages32
JournalMonthly Notices of the Royal Astronomical Society
Volume478
Issue number2
DOIs
Publication statusPublished - 2018

Keywords

  • X, rays
  • catalogs
  • galaxies
  • quasars
  • surveys

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