Galactic Bulge Latitude Survey

Details Galactic Bulge Latitude Survey Galactic Bulge Latitude Survey

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.2067g&link_type=abstract

Chandra Proposal ID #07620944

Computer Science

Chandra Proposal Id #07620944

Scientific paper

Our ChaMPlane and IR program to identify the X-ray sources in the inner bulge has shown these are not dominated by HMXBs. We propose a wide-area multiwavelength survey of the inner galactic bulge, in the latitude direction. We chose the intermediate extinction region at b=-0.2 to -1.5 deg, l=0 deg in order to measure the radial distribution of X-ray point sources out to our deep Chandra survey of selected low extinction windows in the bulge, and provide a comparison for the longitude survey in the bulge plane conducted by Wang et al (2002). Infrared and optical imaging down to the confusion limit will enable a sensitive search for the counterparts despite varying extinction across the field and will extend the logN-logS analysis for the deeper Bulge Chandra fields.

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