C.-T.J. Chen
The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field
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.; Häu\ssler, B.; Norris, R.P.; Silverman, J.D.; Trump, J.R.
Authors
W.N. Brandt
B. Luo
P. Ranalli
G. Yang
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
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
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
M. Sun
M. Tanaka
M. Vaccari
C. Vignali
Y.Q. Xue
M. Banerji
K.E. Chow
B. Häu\ssler
R.P. Norris
J.D. Silverman
J.R. Trump
Abstract
We present an X-ray point-source catalogue from the XMM-Large Scale Structure (XMM-LSS) 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.
Citation
Chen, C.-T., Brandt, W., Luo, B., Ranalli, P., Yang, G., Alexander, D., Bauer, F., Kelson, D., Lacy, M., Nyland, K., Tozzi, P., Vito, F., Cirasuolo, M., Gilli, R., Jarvis, M., Lehmer, B., Paolillo, M., Schneider, D., Shemmer, O., Smail, I., …Trump, J. (2018). The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field. Monthly Notices of the Royal Astronomical Society, 478, 2132-2163. https://doi.org/10.1093/mnras/sty1036
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 20, 2018 |
Online Publication Date | Apr 25, 2018 |
Publication Date | Apr 25, 2018 |
Deposit Date | Jun 28, 2018 |
Publicly Available Date | Jun 29, 2018 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 478 |
Pages | 2132-2163 |
DOI | https://doi.org/10.1093/mnras/sty1036 |
Public URL | https://durham-repository.worktribe.com/output/1327938 |
Publisher URL | http://adsabs.harvard.edu/abs/2018MNRAS.478.2132C |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Authors.
Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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