Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/11362
Title: The first XMM-newton slew survey catalogue: XMMSL1
Authors: Saxton, R. D.
Read, A. M.
Esquej, P.
Freyberg, M. J.
Altieri, B.
Bermejo, D.
First Published: Mar-2008
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy & Astrophysics, 2008, 480 (2), pp. 611-622
Abstract: Aims.We report on the production of a large area, shallow, sky survey, from XMM-Newton slews. The great collecting area of the mirrors coupled with the high quantum efficiency of the EPIC detectors have made XMM-Newton the most sensitive X-ray observatory flown to date. We use data taken with the EPIC-pn camera during slewing manoeuvres to perform an X-ray survey of the sky. Methods. Data from 218 slews have been subdivided into small images and source searched. This has been done in three distinct energy bands; a soft (0.2-2 keV) band, a hard (2-12 keV) band and a total XMM-Newton band (0.2-12 keV). Detected sources, have been quality controlled to remove artifacts and a catalogue has been drawn from the remaining sources. Results.A "full" catalogue, containing 4710 detections and a "clean" catalogue containing 2692 sources have been produced, from 14% of the sky. In the hard X-ray band (2-12 keV) 257 sources are detected in the clean catalogue to a flux limit of 4$\times$10-12 ergs s-1 cm-2. The flux limit for the soft (0.2-2 keV) band is 6$\times$10-13 ergs s-1 cm-2 and for the total (0.2-12 keV) band is 1.2$\times$10-12 ergs s-1 cm-2. The source positions are shown to have an uncertainty of 8´´ (1$\sigma$ confidence).
DOI Link: 10.1051/0004-6361:20079193
ISSN: 0004-6361
Links: http://hdl.handle.net/2381/11362
http://www.aanda.org/articles/aa/abs/2008/11/aa9193-07/aa9193-07.html
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2008 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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