XMM-Newton Proposal 02015006

Details XMM-Newton Proposal 02015006 XMM-Newton Proposal 02015006

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...80c&link_type=abstract

XMM-Newton Proposal ID #02015006

Mathematics

Probability

Ax J1600.5-5143, Ax J1853.5-0103, Ax J1853.3-0128, Ax J1740.2-2904, Ax J1817.6-2401, Ax J1739.2-2923, Xmm-Newton Proposal 02015006

Scientific paper

Discoveries of rotation-powered X-ray pulsars have increased substantially in the last several years, but their properties have yet to conform to a single pattern. We argue that pulsars have a high probability of being found in the vicinity of supernova remnants. Based on a survey of point-like sources in the ASCA archives we propose to use the EPIC-pn detector to investigate new pulsar candidates. The discoveries will fill out the incomplete sample of observed X-ray pulsars, as well as confirm the utility of our method for selecting pulsar candidates from existing archived data.

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