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   72052
   We are completing a survey of the bright Galactic sources detected
   above 1 GeV. We propose here to observe two gamma-ray sources in the
   Cygnus region. With the spectral constraints from the ASCA data and
   archival radio data we will be able to identify AGN seen through the
   plane and pulsar wind nebula candidates for the GeV source
   counterparts. The exposures proposed here and to the Japanese TAC will
   complete a flux-limited search of the Galactic GeV sources and provide
   an important probe of the unidentified gamma-ray population.
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