Overview Science Goals ApJ Intro paper Appendix Team and contacts Publications and Presentations Papers Talks Posters Rapid Release Chandra Survey Selection Criteria Fields Observed NOAO Survey Fields Observed Data Archive X-ray Database Optical Database DS9 Virtual Observatory Quantile Analysis Chandra pointings for ChaMPane Bulge Windows Survey Bulge Latitude Survey Internal Related Links The ChaMPlane survey is being conducted at the Harvard-Smithsonian Center for Astrophysics.

Science Goals The primary goal of ChaMPlane is to identify Cataclysmic Variables (CVs) and quiescent Low Mass X-ray Binaries (qLMXBs: which includes both black hole and neutron star systems), in order to constrain and ultimately measure their number and space density luminosity functions. Secondary objectives are to determine the Be X-ray binary (BeHMXB) content and stellar coronal source distributions in the Galaxy.