Observations of the 100 MeV gamma-ray sources at energies of 100-1000 G eV

Details Observations of the 100 MeV gamma-ray sources at energies of 100-1000 G eV Observations of the 100 MeV gamma-ray sources at energies of 100-1000 G eV

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977esasp.124...39w&link_type=abstract

In ESA Recent Advan. in Gamma-Ray Astronomy p 39-43 (SEE N78-11899 02-88)

Astronomy and Astrophysics

Astronomy

9

Astronomical Observatories, Gamma Rays, Radiation Sources, Atmospheric Radiation, Cerenkov Radiation, Galactic Radiation, Pulsars, Reflecting Telescopes, Sky Surveys (Astronomy)

Scientific paper

Of the sources of gamma rays at energies of 70 MeV discovered by the SAS-2 and COS-B groups, eight were observed with the 10 m reflector on Mt. Hopkins in southern Arizona. All of the observations were in the winter of 1976/7. Because of the positional uncertainty of many of the sources, the detector configuration used was a modified version of that used in the recent high energy Sky Survey. Drift-scans were made on the following sources: (136 deg, + 1 deg), (196 deg, + 4 deg), (120 deg, 0 deg), (98 deg, 0 deg), (187 deg, 0 deg), (175 deg, -5 deg), and (78 deg, 1 deg). The latter scans also included the position of Cyg X-3. At the sensitivity achieved in these observations, none of these sources gave a detectable high energy gamma ray flux.

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