Chandra follow-up of weak persistent sources

Details Chandra follow-up of weak persistent sources Chandra follow-up of weak persistent sources

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2711k&link_type=abstract

Chandra proposal ID #10400048

Physics

Scientific paper

We propose to obtain short exposures of a sample of unclassified sources which are likely weak persistent X-ray binaries. The unique Chandra positional capabilities will allow for an optical follow-up study. Follow-up observations are of paramount importance for the classification of the sources (e.g. as HMXBs/LMXBs, pulsars or in a few rare cases as AXP or DIM). The ACIS sensitivity for hard sources is best while pile-up is no major concern for source localization.

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