A low energy gamma ray observation of the region containing CG 195+4

Details A low energy gamma ray observation of the region containing CG 195+4 A low energy gamma ray observation of the region containing CG 195+4

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...117...38b&link_type=abstract

Astronomy and Astrophysics, vol. 117, no. 1, Jan. 1983, p. 38-40. Research supported by the Science Research Council of England

Astronomy and Astrophysics

Astronomy

4

Gamma Ray Astronomy, Pulsars, Balloon-Borne Instruments, Cos-B Satellite, Gamma Ray Telescopes, Periodic Variations, Statistical Analysis

Scientific paper

During a balloon flight on 8th October 1978, the MISO low energy γ-ray telescope studied the region of sky containing the high energy γ-ray source CG 195+4. No statistically significant fluxes of high energy X-rays or low energy γ-rays in the range 20 keV to 25 MeV were detected, and a search of the data for the 59 s periodicity reported at higher energies gave a negative result.

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