Manners, J.C. and Johnson, O. and Almaini, O. and Willott, C.J. and Gonzalez-Solares, E. and Lawrence, A. and Mann, R.G. and Perez-Fournon, I. and Dunlop, J.S. and McMahon, R.G. and Oliver, S.J. and Rowan-Robinson, M. and Serjeant, S. (2003) The ELAIS deep X-ray survey - I. Chandra source catalogue and first results. Monthly Notices of the Royal Astronomical Society, 343 (1). pp. 293-305. ISSN 0035-8711.
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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.
|Additional information:||35 BLACKWELL PUBLISHING LTD 700JE|
|Uncontrolled keywords:||catalogues; surveys; galaxies : active; X-rays : diffuse background; X-rays : galaxies; X-rays : general ACTIVE GALACTIC NUCLEI; FIELD NORTH SURVEY; N-LOG S; SPECTRAL PROPERTIES; SCUBA-8-MJY SURVEY; OPTICAL SURVEY; LOCKMAN HOLE; ROSAT SURVEY; SUBMILLIMETER; SOUTH|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences|
|Depositing User:||Maggie Francis|
|Date Deposited:||10 Sep 2008 12:34|
|Last Modified:||14 Jan 2010 14:47|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/11793 (The current URI for this page, for reference purposes)|
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