EGRET observations of a mid-latitude region: 10(deg) < b(II) < 45(deg) , -90(deg) < l(II) < 90(deg)

Details EGRET observations of a mid-latitude region: 10(deg) < b(II) < 45(deg) , -90(deg) < l(II) < 90(deg) EGRET observations of a mid-latitude region: 10(deg) < b(II) < 45(deg) , -90(deg) < l(II) < 90(deg)

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.3308n&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #33.08; Bulletin of the American Astronomical Society, Vol. 25, p.847

Astronomy and Astrophysics

Astronomy

Scientific paper

During the Compton Observatory survey of the sky in 1991-92, the EGRET high-energy gamma ray telescope observed this region several times. We will present a synoptic description of the region with particular attention to the point sources observed and their variability. At such moderate galactic latitudes the galactic diffuse background is an important factor, but it does not dominate the point sources as it does nearer the galactic plane. We will compare the theoretical model of the diffuse emission with the observations.

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