The ROSAT wide field camera extragalactic survey

被引:14
作者
Edelson, R [1 ]
Vaughan, S
Warwick, R
Puchnarewicz, E
George, I
机构
[1] Univ Leicester, Dept Phys & Astron, Xray Astron Grp, Leicester LE1 7RH, Leics, England
[2] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[3] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[4] NASA, Goddard Space Flight Ctr, High Energy Astrophys Lab, Greenbelt, MD 20771 USA
[5] Univ Space Res Assoc, Washington, DC USA
关键词
surveys; galaxies : active; BL Lacertae objects : general; galaxies : Seyfert; ultraviolet : galaxies; X-rays : galaxies;
D O I
10.1046/j.1365-8711.1999.02628.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the results of a new analysis of the ROSAT Wide Field Camera (WFC) all-sky survey data, designed to detect extragalactic sources of extreme ultraviolet (EW) radiation in regions of low Galactic N-H. We identify a total of 19 active galactic nuclei (AGN), more than double the number of confirmed AGN in the published WFC (2RE) survey. Our sample contains eight narrow-line Seyfert 1 galaxies, making this the first reasonably sized, complete sample of these extreme AGN, along with six broad-line Seyfert 1s and five BL Lacertae objects. These EUV-selected sources typically have steep soft X-ray spectra with a mean power-law energy index alpha(X) approximate to -2. The derived AGN luminosity function is rather flat and appears to cut off above a luminosity of 10(46) erg s(-1) kev(-1), measured monochromatically at 200 eV. Narrow-line Seyfert Is account for roughly half of the local (z approximate to 0) volume emissivity in the EW band.
引用
收藏
页码:91 / 98
页数:8
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