dc.contributor.author |
Ni, Qingling |
|
dc.contributor.author |
Brand, W. N |
|
dc.contributor.author |
Chen, Chien-Ting |
|
dc.contributor.author |
Luo, Bin |
|
dc.contributor.author |
Nyland, Kristina |
|
dc.contributor.author |
Yang, Guang |
|
dc.contributor.author |
Zou, Fan |
|
dc.contributor.author |
Aird, James |
|
dc.contributor.author |
Alexander, David M |
|
dc.contributor.author |
Bauer, Franz Erik |
|
dc.contributor.author |
Lacy, Mark |
|
dc.contributor.author |
Lehmer, Bret D |
|
dc.contributor.author |
Mallick, Labani |
|
dc.contributor.author |
Salvato, Mara |
|
dc.contributor.author |
Schneider, Donald P |
|
dc.contributor.author |
Tozzi, Paolo |
|
dc.contributor.author |
Traulsen, Iris |
|
dc.contributor.author |
Vaccari, Mattia |
|
dc.contributor.author |
Vignali, Cristian |
|
dc.contributor.author |
Vito, Fabio |
|
dc.contributor.author |
Xue, Yongquan |
|
dc.contributor.author |
Banerji, Manda |
|
dc.contributor.author |
Chow, Kate |
|
dc.contributor.author |
Comastri, Andrea |
|
dc.contributor.author |
Del Moro, Agnese |
|
dc.contributor.author |
Gilli, Roberto |
|
dc.contributor.author |
Mullaney, James |
|
dc.contributor.author |
Paolillo, Maurizio |
|
dc.contributor.author |
Schwope, Axel |
|
dc.contributor.author |
Shemmer, Ohad |
|
dc.contributor.author |
Sun, Mouyuan |
|
dc.contributor.author |
Timlin III, John D |
|
dc.contributor.author |
Trump, Jonathan R |
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dc.date.accessioned |
2021-09-24T15:34:55Z |
|
dc.date.available |
2021-09-24T15:34:55Z |
|
dc.date.issued |
2021-09 |
|
dc.identifier.citation |
The Astrophysical Journal Supplement Series, Vol. 256, No. 1, 21 |
en_US |
dc.identifier.issn |
1538-4365 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/7860 |
|
dc.description |
Restricted Access |
en_US |
dc.description.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. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
IOP Publishing |
en_US |
dc.relation.uri |
https://doi.org/10.3847/1538-4365/ac0dc6 |
|
dc.rights |
© The American Astronomical Society |
|
dc.subject |
Catalogs |
en_US |
dc.subject |
Surveys |
en_US |
dc.subject |
Active galactic nuclei |
en_US |
dc.subject |
Active galaxies |
en_US |
dc.subject |
X-ray active galactic nuclei |
en_US |
dc.subject |
X-ray point sources |
en_US |
dc.subject |
X-ray quasars |
en_US |
dc.subject |
X-ray surveys |
en_US |
dc.title |
The XMM-SERVS Survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields |
en_US |
dc.type |
Article |
en_US |