  Many EHB stars have been found in short-period binaries, where the companions
in these post-common envelope systems are either white dwarfs or dM stars;
these systems are catalogued as hot subdwarfs because the subdwarf is the more
luminous component. Hypothesized Roche-lobe overflow systems (with more massive
companions) may largely be uncatalogued, since the G band or Ca II K-line from
the companion may have caused them to be overlooked or discarded. In
particular, many candidate objects were excluded from the PG catalog because of
such spectroscopic indicators. Could these rejects include large numbers of
"missing" hot subdwarfs? We have examined 2MASS, SDSS, and GALEX archival data
for large subsets of these rejected stars, and conclude that only a handful
(about 3%) show indications of binarity; most are consistent with (single)
metal-poor F stars, as was originally supposed.
