The XMM-SERVS survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields
Q. Ni, W. N. Brandt, C.-T. Chen, B. Luo, K. Nyland, G. Yang, F. Zou,, J. Aird, D. M. Alexander, F. E. Bauer, M. Lacy, B. D. Lehmer, L. Mallick, M., Salvato, D. P. Schneider, P. Tozzi, I. Traulsen, M. Vaccari, C. Vignali, F., Vito, Y. Xue, M. Banerji, K. Chow, A. Comastri

TL;DR
This paper presents X-ray point-source catalogs for two large extragalactic fields from the XMM-SERVS survey, providing extensive data on sources, counterparts, and redshifts to support AGN research.
Contribution
It offers the first comprehensive X-ray source catalogs for the W-CDF-S and ELAIS-S1 fields, including multiwavelength counterparts and redshift information, completing the XMM-SERVS survey.
Findings
Over 6,700 sources detected across both fields.
High identification rates of optical-to-IR counterparts (~87-89%).
Approximately 12,000 sources in the full XMM-SERVS survey.
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 deg) and ELAIS-S1 (3.2 deg), 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 10 erg cm s 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 erg cm s 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…
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