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   PR # 42072
   The nature of the unidentified galactic gamma-ray point sources is
   one of the outstanding puzzles from the EGRET sky survey. The
   singular pulsar Geminga, a very bright gamma-ray source whose nature
   was discovered through X-ray observations, may be the key to
   understanding the constant EGRET point sources. We propose a deep
   survey of several sources near the galactic plane which have
   relatively flat spectra, small EGRET error boxes, and a low
   variability index. By analysing the resultant flux, spectra, and
   morphology we will be able to determine if these sources are
   consistent with the Geminga model, or whether they represent an
   entirely new class of objects.
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