Completing the Galactic Bulge Latitude Survey (BLS)

Computer Science

Scientific paper

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Scientific paper

We propose to complete the Chandra Bulge Latitude Survey (BLS) of +/-1.5deg galactic latitude and +/-0.8deg in longitude about the Galactic Center. The BLS has already shown how the X-ray binary content of the Galactic Center Region matches on to that around the nucleus itself with the cycle 7 and 8 coverage obtained (cycle 9 data not yet obtained). The full survey will be analyzed for source spectra and variability and their distributions about the galactic center. IR photometry (JHK) will be completed with ISPI and optical imaging with Mosaic at the CTIO-4m for the full BLS region to constrain the identifications and nature of the sources. The BLS will provide a Chandra Legacy mosaic image and dataset for comparison with complementary surveys in the inner Galactic Bulge.

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