J.R. Mattox, D.L. Bertsch, C.E. Fichtel, R.C. Hartman, S.D. Hunter, D.J. Thompson, (NASA/GSFC), B.L. Dingus, P. Sreekumar (USRA/GSFC), G. Kanbach, H.A. Mayer-Hasselwander, C. von Montigny (MPE), Y.C. Lin, P.F. Michelson, P.L. Nolan (Stanford), D.A. Kniffen (Hampden-Sydney), E.J. Schneid (Grumman)
The Energetic Gamma Ray Experiment Telescope (EGRET) aboard the
Compton Gamma Ray Observatory detects many point sources
within 10^\circ$ of the Galactic Plane at
longitudes 60^\circ < l <125^\circ$. Analysis has been done
using maximum likelihood and
a model of the diffuse galactic emission (Hunter et al.
conference). A catalog for this region of the sky is presented
which includes information on
energy spectra, time variability, and positions and
position uncertainties. Potential
identifications of some sources are discussed.