The ROSAT north ecliptic pole survey:: The X-ray catalog

被引:62
作者
Henry, JP
Mullis, CR
Voges, W
Böhringer, H
Briel, UG
Gioia, IM
Hochra, JP
机构
[1] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[2] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[3] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[4] CNR, Ist Radioastron INAF, I-40129 Bologna, Italy
[5] Harvard Smithsonian Ctr Astrophys, Salem, MA 01970 USA
关键词
galaxies : active; galaxies : clusters : general; surveys; X-rays : galaxies : clusters; X-rays : general; X-rays : stars;
D O I
10.1086/498749
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The sky around the north ecliptic pole (NEP), at alpha(J2000.0) 18(h)00(m)00(s), delta(J2000.0) = +66 degrees 33'39", has the deepest exposure of the entire ROSAT All-Sky Survey (RASS). The NEP is an undistinguished region of moderate Galactic latitude, b = 29.degrees 8, and hence suitable for compiling statistical samples of both Galactic and extragalactic objects. We have made such a compilation in the 80.6 deg(2) region surrounding the NEP. Our sample fully exploits the properties of the RASS, since the only criteria for inclusion are source position and significance, and it yields the deepest large solid angle contiguous sample of X-ray sources to date. We find 442 unique sources above a flux limit similar to 2; 10(-14) ergs cm(-2) s(-1) in the 0.5-2.0 keV band. In this paper we present the X-ray properties of these sources as determined from the RASS. These include positions, fluxes, spectral information in the form of hardness ratios, and angular sizes. Since we have performed a comprehensive optical identification program we also present the average X-ray properties of classes of objects typical of the X-ray sky at these flux levels. We discuss the use of the RASS to find clusters of galaxies based on their X-ray properties alone.
引用
收藏
页码:304 / 328
页数:25
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