The ELAIS deep X-ray survey -: I.: Chandra source catalogue and first results

被引:66
|
作者
Manners, JC
Johnson, O
Almaini, O
Willott, CJ
Gonzalez-Solares, E
Lawrence, A
Mann, RG
Perez-Fournon, I
Dunlop, JS
McMahon, RG
Oliver, SJ
Rowan-Robinson, M
Serjeant, S
机构
[1] Univ Edinburgh, Astron Inst, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland
[2] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[3] Univ Sussex, Ctr Astron, CPES, Brighton BN1 9QJ, E Sussex, England
[4] Inst Astrofis Canarias, Tenerife 38200, Spain
[5] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[6] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2BW, England
[7] Univ Kent, Unit Space Sci & Astrophys, Sch Phys Sci, Canterbury CT2 7NZ, Kent, England
关键词
catalogues; surveys; galaxies : active; X-rays : diffuse background; X-rays : galaxies; X-rays : general;
D O I
10.1046/j.1365-8711.2003.06672.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an analysis of two deep (75 ks) Chandra observations of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) fields N1 and N2 as the first results from the ELAIS deep X-ray survey. This survey is being conducted in well-studied regions with extensive multiwavelength coverage. Here we present the Chandra source catalogues along with an analysis of source counts, hardness ratios and optical classifications. A total of 233 X-ray point sources are detected in addition to two soft extended sources, which are found to be associated with galaxy clusters. An overdensity of sources is found in N1 with 30 per cent more sources than N2, which we attribute to large-scale structure. A similar variance is seen between other deep Chandra surveys. The source count statistics reveal an increasing fraction of hard sources at fainter fluxes. The number of galaxy-like counterparts also increases dramatically towards fainter fluxes, consistent with the emergence of a large population of obscured sources.
引用
收藏
页码:293 / 305
页数:13
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