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The population of stellar black holes (SBHs) in the Galaxy and galaxiesgenerally is poorly known in both number and distribution. SBHs are the fossilrecord of the massive stars in galaxy evolution and may have produced some (ifnot all) of the intermediate mass (\gsim100\Msun) black holes (IMBHs) and, inturn, the central supermassive black holes (SMBHs) in galactic nuclei. For thefirst time, a Galaxy-wide census of accreting black holes, and their morereadily recognizable tracer population, accreting neutron stars (NSs), could bemeasured with a wide-field hard X-ray imaging survey and soft X-ray andoptical/IR prompt followup -- as proposed for the EXIST mission.

Measuring the Accreting Stellar and Intermediate Mass Black Hole Populations in the Galaxy and Local Group