EGRET Observations of High-Energy Gamma Rays from Geminga

Details EGRET Observations of High-Energy Gamma Rays from Geminga EGRET Observations of High-Energy Gamma Rays from Geminga

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...18111203n&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #112.03; Bulletin of the American Astronomical Society, Vol. 24, p.1299

Astronomy and Astrophysics

Astronomy

Scientific paper

The EGRET high-energy gamma ray telescope on the Compton Gamma Ray Observatory satellite (CGRO) observed the gamma-ray pulsar Geminga three times in 1991 and five times (albeit with low sensitivity) in 1992. A new ephemeris has been derived, based on the EGRET data alone. Phase-resolved spectra for the 30-10000 MeV energy range have been derived for the two peaks, the interpulse interval, and the ``extrapulse'' interval.

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