Physics – Optics
Scientific paper
May 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cuny.reptr....h&link_type=abstract
Annual Status Report, 15 Feb. 1994 - 14 Feb. 1995 Columbia Univ., New York, NY. Dept. of Astronomy and Physics.
Physics
Optics
Gamma Ray Astronomy, Gamma Ray Spectra, Gamma Ray Telescopes, Gamma Rays, Pulsars, Radio Astronomy, Radio Sources (Astronomy), Wavelengths, X Ray Astronomy, X Ray Spectra, Astronomical Catalogs, Data Correlation, Data Processing, Data Reduction, Gamma Ray Observatory, X Ray Optics
Scientific paper
As was the case for COS B, the majority of high-energy (greater than 100 MeV) gamma-ray sources detected by the EGRET instrument on GRO are not immediately identifiable with catalogued objects at other wavelengths. These persistent gamma-ray sources are, next to the gamma-ray bursts, the least understood objects in the universe. This two year investigation is intended to support the analysis, correlation, and theoretical interpretation of data that we are obtaining at x-ray, optical, and radio wavelengths in order to render the gamma-ray data interpretable. This second year was devoted to studies of unidentified gamma-ray sources from the first EGRET catalog, similar to previous observations. Efforts have concentrated on the sources at low and intermediate Galactic latitudes, which are the most plausible pulsar candidates.
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