Galactic Bulge Chandra-HST Survey

Details Galactic Bulge Chandra-HST Survey Galactic Bulge Chandra-HST Survey

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1824g&link_type=abstract

Chandra Proposal ID #06620985

Computer Science

Chandra Proposal Id #06620985

Scientific paper

We propose a deep survey for low luminosity accretion powered sources (CVs, qLMXBs and wind-fed pulsars) that likely constitute the underlying populations in the cusp of sources around SgrA*. A 100ksec pointing at l,b = 0.10, -1.43 allows the survey closest to the galactic center that can still be reached in optical. With 12 orbits of HST, we can complement the two outer fields (Baade's Window and Stanek Window) obtained with Chandra-HST to complete the most sensitive X-ray/optical survey of the Galactic Bulge.

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