The XMM-SERVS survey:: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields

Qingling Ni; W. N. Brandt; Chien-ting Chen; Bin Luo; Kristina Nyland; Guang Yang; Fan Zou; James Aird; David M. Alexander; 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 III; Jonathan R. Trump

doi:10.3847/1538-4365/ac0dc6

The XMM-SERVS survey: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields

Qingling Ni^*, W. N. Brandt, Chien-ting Chen, Bin Luo, Kristina Nyland, Guang Yang, Fan Zou, James Aird, David M. Alexander, Franz Erik Bauer, Mark Lacy, Bret D. Lehmer, Labani Mallick, Mara Salvato, Donald P. Schneider, Paolo Tozzi, Iris Traulsen, Mattia Vaccari, Cristian Vignali, Fabio VitoYongquan 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 III, Jonathan R. Trump

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

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-S1regions 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 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 ≈ 89% of the sources in W-CDF-S and ≈ 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; ≈ 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 ≈ 12,000 point-like X-ray sources detected in the whole ≈ 13 deg2 XMM-SERVS survey will benefit future large-sample AGN studies.

Original language	English
Article number	21
Journal	Astrophysical Journal Supplement
Volume	256
Issue number	1
DOIs	https://doi.org/10.3847/1538-4365/ac0dc6
Publication status	Published - 14 Sept 2021

Keywords / Materials (for Non-textual outputs)

astro-ph.GA

Access to Document

10.3847/1538-4365/ac0dc6

2106.10572v1Accepted author manuscript, 9.77 MB

Connecting the lifecycles of galaxies and their central black holes
Aird, J. & Best, P.
Other
1/11/20 → 31/10/24
Project: Research

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Ni, Q., Brandt, W. N., Chen, C., 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., ... 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

@article{e1f6d1d117b7484ba913b6d8502e238d,

title = "The XMM-SERVS survey:: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields",

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-S1regions 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 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 ≈ 89% of the sources in W-CDF-S and ≈ 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; ≈ 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 ≈ 12,000 point-like X-ray sources detected in the whole ≈ 13 deg2 XMM-SERVS survey will benefit future large-sample AGN studies.",

keywords = "astro-ph.GA",

author = "Qingling Ni and Brandt, {W. N.} and Chien-ting Chen and Bin Luo and Kristina Nyland and Guang Yang and Fan Zou and James Aird and Alexander, {David M.} and Bauer, {Franz Erik} and Mark Lacy and Lehmer, {Bret D.} and Labani Mallick and Mara Salvato and Schneider, {Donald P.} and Paolo Tozzi and Iris Traulsen and Mattia Vaccari and Cristian Vignali and Fabio Vito and Yongquan Xue and Manda Banerji and Kate Chow and Andrea Comastri and {Del Moro}, Agnese and Roberto Gilli and James Mullaney and Maurizio Paolillo and Axel Schwope and Ohad Shemmer and Mouyuan Sun and {Timlin III}, {John D.} and Trump, {Jonathan R.}",

note = "*Awaiting pub date before adding 12 month embargo dates.* 40 pages, 35 figures. Accepted for publication in ApJS. Data products available at: https://personal.psu.edu/wnb3/xmmservs/xmmservs.html",

year = "2021",

month = sep,

day = "14",

doi = "10.3847/1538-4365/ac0dc6",

language = "English",

volume = "256",

journal = "Astrophysical Journal Supplement",

issn = "0067-0049",

publisher = "IOP Publishing",

number = "1",

}

Ni, Q, Brandt, WN, Chen, C, Luo, B, Nyland, K, Yang, G, Zou, F, Aird, J, Alexander, DM, Bauer, FE, Lacy, M, Lehmer, BD, Mallick, L, Salvato, M, Schneider, DP, Tozzi, P, Traulsen, I, Vaccari, M, Vignali, C, Vito, F, Xue, Y, Banerji, M, Chow, K, Comastri, A, Del Moro, A, Gilli, R, Mullaney, J, Paolillo, M, Schwope, A, Shemmer, O, Sun, M, Timlin III, JD & Trump, JR 2021, 'The XMM-SERVS survey: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields', Astrophysical Journal Supplement, vol. 256, no. 1, 21. https://doi.org/10.3847/1538-4365/ac0dc6

TY - JOUR

T1 - The XMM-SERVS survey:

T2 - XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields

AU - Ni, Qingling

AU - Brandt, W. N.

AU - Chen, Chien-ting

AU - Luo, Bin

AU - Nyland, Kristina

AU - Yang, Guang

AU - Zou, Fan

AU - Aird, James

AU - Alexander, David M.

AU - Bauer, Franz Erik

AU - Lacy, Mark

AU - Lehmer, Bret D.

AU - Mallick, Labani

AU - Salvato, Mara

AU - Schneider, Donald P.

AU - Tozzi, Paolo

AU - Traulsen, Iris

AU - Vaccari, Mattia

AU - Vignali, Cristian

AU - Vito, Fabio

AU - Xue, Yongquan

AU - Banerji, Manda

AU - Chow, Kate

AU - Comastri, Andrea

AU - Del Moro, Agnese

AU - Gilli, Roberto

AU - Mullaney, James

AU - Paolillo, Maurizio

AU - Schwope, Axel

AU - Shemmer, Ohad

AU - Sun, Mouyuan

AU - Timlin III, John D.

AU - Trump, Jonathan R.

N1 - *Awaiting pub date before adding 12 month embargo dates.* 40 pages, 35 figures. Accepted for publication in ApJS. Data products available at: https://personal.psu.edu/wnb3/xmmservs/xmmservs.html

PY - 2021/9/14

Y1 - 2021/9/14

N2 - 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-S1regions 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 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 ≈ 89% of the sources in W-CDF-S and ≈ 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; ≈ 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 ≈ 12,000 point-like X-ray sources detected in the whole ≈ 13 deg2 XMM-SERVS survey will benefit future large-sample AGN studies.

AB - 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-S1regions 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 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 ≈ 89% of the sources in W-CDF-S and ≈ 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; ≈ 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 ≈ 12,000 point-like X-ray sources detected in the whole ≈ 13 deg2 XMM-SERVS survey will benefit future large-sample AGN studies.

KW - astro-ph.GA

U2 - 10.3847/1538-4365/ac0dc6

DO - 10.3847/1538-4365/ac0dc6

M3 - Article

SN - 0067-0049

VL - 256

JO - Astrophysical Journal Supplement

JF - Astrophysical Journal Supplement

IS - 1

M1 - 21

ER -

The XMM-SERVS survey: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields

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Keywords / Materials (for Non-textual outputs)

Access to Document

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Connecting the lifecycles of galaxies and their central black holes

Cite this