XMM observations of the Lockman Hole (Brunner+, 2008)

Details XMM observations of the Lockman Hole (Brunner+, 2008) XMM observations of the Lockman Hole (Brunner+, 2008)

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34790283b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/479/283. Originally published in: 2008A&A...479..283B

Physics

X-Ray Sources, Surveys, Positional Data

Scientific paper

The Lockman Hole represents the sky area of lowest Galactic line-of-sight columns density. It was observed by the XMM-Newton X-ray observatory in 18 pointings performed between April 2000 and December 2002. The total exposure time spent on the field was 1.16Ms (EPIC pn detector; EPIC MOS detector: 1.30 Ms). The effective exposure after removal of times of high particle background is 637ks (EPIC pn detector; EPIC MOS detector: 765ks). The catalogue lists positions, count rates, fluxes, hardness ratios, and partial optical classifications of 409 X-ray point sources detected in the central 0.196{deg}2 of the field down to a detection likelihood threshold of 10 (3.9sigma). The analysis was performed using the XMM-Newton SAS data analysis package version 6.0.
(1 data file).

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