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Table 2: The number of sources from each of the major classes detected by ISGRI are listed for new ( $\equiv$ IGRs) and previously-known sources. Miscellaneous (Misc.) sources are Galactic objects that are not X-ray binaries (e.g. CVs, SNRs, AXPs, etc.) and Uncl. refers to the group of sources that have yet to be classified.
Table 3: Parameters from the model described in the text fit to the distributions of scale heights from the Galactic plane for HMXBs, LMXBs and miscellaneous sources whose distances are known. Objects from the Magellanic Clouds are excluded.
Table 1: The parameters of sources detected by ISGRI.