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Paper
The XMM-SERVS survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields
2021
Overview
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 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 Ms and 1.0 Ms of XMM-Newton observations, respectively; 1.8 Ms and 0.9 Ms exposures remain after flare filtering. The survey in W-CDF-S has a flux limit of 1.0 \\(\\times\\) 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 \\(\\times\\) 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 \\(\\approx\\) 89% of the sources in W-CDF-S and \\(\\approx\\) 87% of the sources in ELAIS-S1. 3186 sources in W-CDF-S and 1985 sources in ELAIS-S1 are classified as AGNs. We also provide photometric redshifts for X-ray sources; \\(\\approx\\) 84% of the 3319/2001 sources in W-CDF-S/ELAIS-S1 with optical-to-NIR 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 \\(\\approx\\) 12,000 point-like X-ray sources detected in the whole \\(\\approx\\) 13 deg\\(^2\\) XMM-SERVS survey will benefit future large-sample AGN studies.
Publisher
Cornell University Library, arXiv.org
Subject
