The Subaru/XMM-Newton Deep Survey (SXDS). III. X-Ray Data
The Subaru/XMM-Newton Deep Survey (SXDS). III. X-Ray Data
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DOI:
10.1086/591083
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发表时间:
2008-06
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影响因子:
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通讯作者:
Y. Ueda;M. Watson;I. Stewart;M. Akiyama;A. Schwope;G. Lamer;J. Ebrero;F. Carrera;K. Sekiguchi-K.-Seki
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文献类型:
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作者:
Y. Ueda;M. Watson;I. Stewart;M. Akiyama;A. Schwope;G. Lamer;J. Ebrero;F. Carrera;K. Sekiguchi-K.-Seki
We present the X-ray source catalog in the Subaru/XMM-Newton deep survey. A continuous area of 1.14 deg2 centered at R .A . = 02h18m and decl . = − 05° is mapped by seven pointings with XMM-Newton covering the 0.2-10 keV band. From the combined images of the EPIC pn and MOS cameras, we detect 866, 1114, 645, and 136 sources with sensitivity limits of 6 × 10−16, 8 × 10−16, 3 × 10−15, and 5 × 10−15 ergs cm−2 s−1 in the 0.5-2, 0.5-4.5, 2-10, and 4.5-10 keV bands, respectively, with detection likelihood ≥7 (corresponding to a confidence level of 99.91%). The catalog consists of 1245 sources in total including 32 extended-source candidates. The averaged log N–log S relations are in good agreement with previous results, bridging the flux range between Chandra deep surveys and brighter surveys. The log N–log S relations show significant spatial variation among pointings on a scale of 0.2 deg2. Analyzing the autocorrelation function, we detect significant clustering signals from the 0.5-2 keV band sample, which can be fit with a power-law form (θ/θc)−0.8 with a correlation length of θc = 5.9+ 1.0−0.9 arcsec when the integral constraint term is included. In the 2-10 keV band, however, the clustering is not significant with a 90% upper limit of θc < 1.5″.