The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields

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dc.contributor.authorNi, Qingling
dc.contributor.authorBrandt, W. N.
dc.contributor.authorChen, Chien-Ting
dc.contributor.authorLuo, Bin
dc.contributor.authorNyland, Kristina
dc.contributor.authorYang, Guang
dc.contributor.authorZou, Fan
dc.contributor.authorAird, James
dc.contributor.authorAlexander, David M.
dc.contributor.authorBauer, Franz Erik
dc.contributor.authorLacy, Mark
dc.contributor.authorLehmer, Bret D.
dc.contributor.authorMallick, Labani
dc.contributor.authorSalvato, Mara
dc.contributor.authorSchneider, Donald P.
dc.contributor.authorTozzi, Paolo
dc.contributor.authorTraulsen, Iris
dc.contributor.authorVaccari, Mattia
dc.contributor.authorVignali, Cristian
dc.contributor.authorVito, Fabio
dc.contributor.authorXue, Yongquan
dc.contributor.authorBanerji, Manda
dc.contributor.authorChow, Kate
dc.contributor.authorComastri, Andrea
dc.contributor.authorDel Moro, Agnese
dc.contributor.authorGilli, Roberto
dc.contributor.authorMullaney, James
dc.contributor.authorPaolillo, Maurizio
dc.contributor.authorSchwope, Axel
dc.contributor.authorShemmer, Ohad
dc.contributor.authorSun, Mouyuan
dc.contributor.authorTimlin III, John D.
dc.contributor.authorTrump, Jonathan R.
dc.date.accessioned2025-01-20T22:08:40Z
dc.date.available2025-01-20T22:08:40Z
dc.date.issued2021
dc.description.abstractWe 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 deg(2)) and ELAIS-S1 (3.2 deg(2)), 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 x 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 x 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 approximate to 89% of the sources in W-CDF-S and approximate to 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; approximate to 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 approximate to 12,000 pointlike X-ray sources detected in the whole approximate to 13 deg(2) XMM-SERVS survey will benefit future large-sample AGN studies.
dc.fuente.origenWOS
dc.identifier.doi10.3847/1538-4365/ac0dc6
dc.identifier.eissn1538-4365
dc.identifier.issn0067-0049
dc.identifier.urihttps://doi.org/10.3847/1538-4365/ac0dc6
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/94306
dc.identifier.wosidWOS:000695281700001
dc.issue.numero1
dc.language.isoen
dc.revistaAstrophysical journal supplement series
dc.rightsacceso restringido
dc.titleThe XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields
dc.typeartículo
dc.volumen256
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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