Galactic Bulge Deep Survey

Computer Science

Scientific paper

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Chandra Proposal Id #05301004

Scientific paper

We propose a deep survey in the second lowest extinction (after Baades Window) region in the galactic bulge, the window identified by Stanek (1998) at l,b ~ 0.25, -2.1. This will complement our deep survey of Baades Window scheduled for cycle 4 and allow comparative source populations, and constraints on the gradient towards the galactic center, to be derived. HST orbits (9) are requested to do the optical identifications in this field down to Mv ~9, sufficient to identify most CVs and qLMXBs. This will constrain the compact object populations in the galactic bulge.

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