The Galactic Bulge Survey: categorising the plethora of faint X-ray sources in the Galactic Bulge

Details The Galactic Bulge Survey: categorising the plethora of faint X-ray sources in the Galactic Bulge The Galactic Bulge Survey: categorising the plethora of faint X-ray sources in the Galactic Bulge

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2316j&link_type=abstract

Chandra Proposal ID #09400196

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Chandra Proposal Id #09400196

Scientific paper

We propose to image an area of 6x1 degrees centered on the Galactic Center at |b|=1.5 degrees: the Galactic Bulge Survey. 25% of this area will be observed as an SRON GTO program in AO9. We here propose for another 25%. These regions have been selected because of their lower extinction and crowding in the optical and near-infrared than in the Galactic Center area, while still having a high density of X-ray sources. We will detect a plethora of faint X-ray sources that will constrain binary evolution models by way of a number count and by identifying predicted X-ray binary types that so far have eluded identification. We expect to find (quiescent) eclipsing neutron star and black hole LMXBs. These are important for neutron star and black hole mass measurements.

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