B. Luo
The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
Luo, B.; Brandt, W.N.; Xue, Y.Q.; Lehmer, B.; Alexander, D.M.; Bauer, F.E.; Vito, F.; Yang, G.; Basu-Zych, A.R.; Comastri, A.; Gilli, R.; Gu, Q.-S.; Hornschemeier, A.E.; Koekemoer, A.; Liu, T.; Mainieri, V.; Paolillo, M.; Ranalli, P.; Rosati, P.; Schneider, D.P.; Shemmer, O.; Smail, I.; Sun, M.; Tozzi, P.; Vignali, C.; Wang, J.-X.
Authors
W.N. Brandt
Y.Q. Xue
B. Lehmer
Professor David Alexander d.m.alexander@durham.ac.uk
Professor
F.E. Bauer
F. Vito
G. Yang
A.R. Basu-Zych
A. Comastri
R. Gilli
Q.-S. Gu
A.E. Hornschemeier
A. Koekemoer
T. Liu
V. Mainieri
M. Paolillo
P. Ranalli
P. Rosati
D.P. Schneider
O. Shemmer
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
M. Sun
P. Tozzi
C. Vignali
J.-X. Wang
Abstract
We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin2. Utilizing wavdetect for initial source detection and ACIS Extract for photometric extraction and significance assessment, we create a main source catalog containing 1008 sources that are detected in up to three X-ray bands: 0.5–7.0 keV, 0.5–2.0 keV, and 2–7 keV. A supplementary source catalog is also provided, including 47 lower-significance sources that have bright (${K}_{s}\leqslant 23$) near-infrared counterparts. We identify multiwavelength counterparts for 992 (98.4%) of the main-catalog sources, and we collect redshifts for 986 of these sources, including 653 spectroscopic redshifts and 333 photometric redshifts. Based on the X-ray and multiwavelength properties, we identify 711 active galactic nuclei (AGNs) from the main-catalog sources. Compared to the previous ≈4 Ms CDF-S catalogs, 291 of the main-catalog sources are new detections. We have achieved unprecedented X-ray sensitivity with average flux limits over the central ≈1 arcmin2 region of ≈1.9 × 10−17, 6.4 × 10−18, and 2.7 × 10−17 erg cm−2 s−1 in the three X-ray bands, respectively. We provide cumulative number-count measurements observing, for the first time, that normal galaxies start to dominate the X-ray source population at the faintest 0.5–2.0 keV flux levels. The highest X-ray source density reaches ≈50,500 deg−2, and 47% ± 4% of these sources are AGNs (≈23,900 deg−2).
Citation
Luo, B., Brandt, W., Xue, Y., Lehmer, B., Alexander, D., Bauer, F., …Wang, J. (2017). The Chandra Deep Field-South Survey: 7 Ms Source Catalogs. Astrophysical Journal Supplement, 228(1), Article 2. https://doi.org/10.3847/1538-4365/228/1/2
Journal Article Type | Article |
---|---|
Acceptance Date | Nov 7, 2016 |
Online Publication Date | Dec 27, 2016 |
Publication Date | Jan 1, 2017 |
Deposit Date | Feb 22, 2017 |
Publicly Available Date | Mar 7, 2017 |
Journal | Astrophysical Journal Supplement |
Print ISSN | 0067-0049 |
Electronic ISSN | 1538-4365 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 228 |
Issue | 1 |
Article Number | 2 |
DOI | https://doi.org/10.3847/1538-4365/228/1/2 |
Public URL | https://durham-repository.worktribe.com/output/1385216 |
Related Public URLs | https://arxiv.org/abs/1611.03501 |
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Copyright Statement
© 2016. The American Astronomical Society. All rights reserved.
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