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

Authors :
Jonathan R. Trump
Ian Smail
Ray P. Norris
Chien-Ting J. Chen
David M. Alexander
Franz E. Bauer
Paolo Tozzi
Kristina Nyland
B. Häußler
Ohad Shemmer
D. D. Kelson
Mouyuan Sun
Matt J. Jarvis
Piero Ranalli
Michele Cirasuolo
John D. Silverman
Maurizio Paolillo
Mark Lacy
W. N. Brandt
Fabio Vito
M. Banerji
Roberto Gilli
Guang Yang
Bret D. Lehmer
Donald P. Schneider
Kate Chow
Yongquan Xue
Mattia Vaccari
Masayuki Tanaka
B. Luo
Cristian Vignali
Chen, C.-T.J.
Brandt, W.N.
Luo, B.
Ranalli, P.
Yang, G.
Alexander, D.M.
Bauer, F.E.
Kelson, D.D.
Lacy, M.
Nyland, K.
Tozzi, P.
Vito, F.
Cirasuolo, M.
Gilli, R.
Jarvis, M.J.
Lehmer, B.D.
Paolillo, M.
Schneider, D.P.
Shemmer, O.
Smail, I.
Sun, M.
Tanaka, M.
Vaccari, M.
Vignali, C.
Xue, Y.Q.
Banerji, M.
Chow, K.E.
Häußler, B.
Norris, R.P.
Silverman, J.D.
Trump, J.R.
Chen, C. -T. J.
Brandt, W. N.
Alexander, D. M.
Bauer, F. E.
Kelson, D. D.
Jarvis, M. J.
Lehmer, B. D.
Schneider, D. P.
Xue, Y. Q.
Chow, K. E.
Norris, R. P.
Silverman, J. D.
Trump, J. R.
ITA
USA
GBR
DEU
JPN
CHN
Source :
Monthly notices of the Royal Astronomical Society, 2018, Vol.478, pp.2132-2163 [Peer Reviewed Journal]
Publication Year :
2018
Publisher :
Oxford University Press, 2018.

Abstract

We present an X-ray point-source catalog from the XMM-Large Scale Structure survey region (XMM-LSS), 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 catalog 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% expected spurious fraction determined from simulations. A total of 2381 new X-ray sources are detected compared to previous source catalogs in the same area. Our survey has flux limits of $1.7\times10^{-15}$, $1.3\times10^{-14}$, and $6.5\times10^{-15}$ erg cm$^{-2}$ s$^{-1}$ over 90% 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% of the X-ray sources, of which 93% are considered as reliable based on their matching likelihood ratios. The reliabilities of these high-likelihood-ratio counterparts are further confirmed to be $\approx 97$% reliable based on deep Chandra coverage over $\approx 5$% of the XMM-LSS region. Results of multiwavelength identifications are also included in the source catalog, 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 deg$^2$ of our field where forced-aperture multi-band photometry is available; $>70$% of the X-ray sources in this subfield have either spectroscopic or high-quality photometric redshifts.<br />MNRAS, accepted. 34 pages, 25 figures, and 8 tables. The data products are available at this http url: http://personal.psu.edu/wnb3/xmmservs/xmmservs.html

Details

Database :
OpenAIRE
Journal :
Monthly notices of the Royal Astronomical Society, 2018, Vol.478, pp.2132-2163 [Peer Reviewed Journal]
Accession number :
edsair.doi.dedup.....1bb1ecb7e83d69eb2e11043905e6fbde