Title: Spatial and Spectral Analysis of COMPTEL Gamma-Ray Bursts Author(s) and Affiliation(s): R.M. Kippen, J. Ryan, A. Connors, M. McConnell (University of New Hampshire), C. Winkler, Astrophysics Division, ESTEC), V. Schoenfelder, J. Greiner, M. Varendorff, W. Collmar (Max-Planck Institut fuer Extraterrestrische Physik), W. Hermsen and L. Kuiper (SRON-Utrecht) Subject Area: Gamma-ray Bursts Abstract: We present results from the spatial and spectral analysis of 27 gamma-ray bursts measured by the COMPTEL ``Telescope'' instrument during four years of observations. Accurate burst locations ($\sim$1$\degr$, 1$\sigma$) and high-energy sensitivity (0.75--30 MeV) allow us to study the small-scale angular source distribution and high-energy spectral characteristics. The COMPTEL burst locations are statistically consistent with an isotropic angular distribution of sources on both large and small angular scales, despite the spatial coincidence of two of the bursts. The time-averaged COMPTEL burst spectra are consistent with a simple power law model above 1 MeV, with spectral indices in the range 1.5--3.5. Measurement of rapid variability at MeV energies in the stronger bursts indicates that that either the sources are nearby (within the Galaxy) or the gamma-ray emission is relativistically beamed. We review recent analysis results obtained with the existing COMPTEL burst catalog and give an update on new observations, including the on going search for fading low-energy counterparts using rapidly-determined COMPTEL burst locations. -eof-