Galactic Bulge Chandra-HST Survey

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

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10353g&link_type=abstract

HST Proposal ID #10353

Computer Science

Hst Proposal Id #10353

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 100 ksec pointing at l, b = 0.10, -1.43 degr. allows the survey closest to the galactic center that can still be reached in the optical. With 12 orbits of HST, we can complement the two outer fields {Baade's Window and Stanek's Window} obtained with Chandra-HST to complete the most sensitive X-ray/optical survey of the Galactic Bulge.

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