Qingling Ni
The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields
Ni, Qingling; Brandt, W.N.; Chen, Chien-Ting; Luo, Bin; Nyland, Kristina; Yang, Guang; Zou, Fan; Aird, James; Alexander, David M.; Bauer, Franz Erik; Lacy, Mark; Lehmer, Bret D.; Mallick, Labani; Salvato, Mara; Schneider, Donald P.; Tozzi, Paolo; Traulsen, Iris; Vaccari, Mattia; Vignali, Cristian; Vito, Fabio; Xue, Yongquan; Banerji, Manda; Chow, Kate; Comastri, Andrea; Del Moro, Agnese; Gilli, Roberto; Mullaney, James; Paolillo, Maurizio; Schwope, Axel; Shemmer, Ohad; Sun, Mouyuan; Timlin, John D.; Trump, Jonathan R.
Authors
W.N. Brandt
Chien-Ting Chen
Bin Luo
Kristina Nyland
Guang Yang
Fan Zou
James Aird
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
Franz Erik Bauer
Mark Lacy
Bret D. Lehmer
Labani Mallick
Mara Salvato
Donald P. Schneider
Paolo Tozzi
Iris Traulsen
Mattia Vaccari
Cristian Vignali
Fabio Vito
Yongquan Xue
Manda Banerji
Kate Chow
Andrea Comastri
Agnese Del Moro
Roberto Gilli
James Mullaney
Maurizio Paolillo
Axel Schwope
Ohad Shemmer
Mouyuan Sun
John D. Timlin
Jonathan R. Trump
Abstract
We present the X-ray point-source catalogs in two of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields, W-CDF-S (4.6 deg2) and ELAIS-S1 (3.2 deg2), aiming to fill the gap between deep pencil-beam X-ray surveys and shallow X-ray surveys over large areas. The W-CDF-S and ELAIS-S1 regions were targeted with 2.3 and 1.0 Ms of XMM-Newton observations, respectively; 1.8 and 0.9 Ms exposures remain after flare filtering. The survey in W-CDF-S has a flux limit of 1.0 × 10−14 erg cm−2 s−1 over 90% of its area in the 0.5–10 keV band; 4053 sources are detected in total. The survey in ELAIS-S1 has a flux limit of 1.3 × 10−14 erg cm−2 s−1 over 90% of its area in the 0.5–10 keV band; 2630 sources are detected in total. Reliable optical-to-IR multiwavelength counterpart candidates are identified for ≈89% of the sources in W-CDF-S and ≈87% of the sources in ELAIS-S1. A total of 3129 sources in W-CDF-S and 1957 sources in ELAIS-S1 are classified as active galactic nuclei (AGNs). We also provide photometric redshifts for X-ray sources; ≈84% of the 3319/2001 sources in W-CDF-S/ELAIS-S1 with optical-to-near-IR forced photometry available have either spectroscopic redshifts or high-quality photometric redshifts. The completion of the XMM-Newton observations in the W-CDF-S and ELAIS-S1 fields marks the end of the XMM-SERVS survey data gathering. The ≈12,000 pointlike X-ray sources detected in the whole ≈13 deg2 XMM-SERVS survey will benefit future large-sample AGN studies.
Citation
Ni, Q., Brandt, W., Chen, C.-T., Luo, B., Nyland, K., Yang, G., Zou, F., Aird, J., Alexander, D. M., Bauer, F. E., Lacy, M., Lehmer, B. D., Mallick, L., Salvato, M., Schneider, D. P., Tozzi, P., Traulsen, I., Vaccari, M., Vignali, C., Vito, F., …Trump, J. R. (2021). The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields. Astrophysical Journal Supplement, 256(1), Article 21. https://doi.org/10.3847/1538-4365/ac0dc6
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 17, 2021 |
Online Publication Date | Sep 14, 2021 |
Publication Date | 2021 |
Deposit Date | Nov 10, 2021 |
Publicly Available Date | Nov 10, 2021 |
Journal | The Astrophysical Journal Supplement Series |
Print ISSN | 0067-0049 |
Electronic ISSN | 1538-4365 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 256 |
Issue | 1 |
Article Number | 21 |
DOI | https://doi.org/10.3847/1538-4365/ac0dc6 |
Public URL | https://durham-repository.worktribe.com/output/1223681 |
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© 2021. The American Astronomical Society. All rights reserved.
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