期刊
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 228, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4365/228/1/2
关键词
catalogs; cosmology: observations; diffuse radiation; galaxies: active; surveys; X-rays: galaxies
资金
- National Thousand Young Talents program of China
- National Natural Science Foundation of China [11673010]
- Ministry of Science and Technology of China [2016YFA0400702]
- CXC [GO4-15130A]
- 973 Program [2015CB857004, 2015CB857005]
- Strategic Priority Research Program of CAS [XDB09000000]
- Fundamental Research Funds for the Central Universities
- CAS Frontier Science Key Research Program [QYZDJ-SSW-SLH006]
- STFC [ST/L00075X/1]
- CONICYT-Chile [Basal-CATA PFB-06/2007]
- FONDECYT [1141218]
- EMBIGGEN Anillo [ACT1101]
- Ministry of Economy, Development, and Tourism's Millennium Science Initiative [IC120009]
- ERC [DUSTYGAL 321334]
- Royal Society/Wolfson Merit Award
- [NSFC-11473026]
- [NSFC-11421303]
- STFC [ST/P000541/1] Funding Source: UKRI
We present X-ray source catalogs for the approximate to 7 Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2. arcmin(2). 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 <= 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 approximate to 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 approximate to 1 arcmin(2) region of approximate to 1.9. x. 10(-17), 6.4 x 10(-18), and 2.7 x 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 approximate to 50,500 deg(-2), and 47% +/- 4% of these sources are AGNs (approximate to 23,900 deg(-2)).
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