Low-energy gamma-ray emission close to CG 135 + 1

Details Low-energy gamma-ray emission close to CG 135 + 1 Low-energy gamma-ray emission close to CG 135 + 1

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239l..49p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 239, July 15, 1980, p. L49-L52. Research supported by the Science Re

Astronomy and Astrophysics

Astronomy

43

Cos-B Satellite, Gamma Ray Astronomy, Photon Density, Quasars, Astronomical Coordinates, Balloon Flight, Radio Sources (Astronomy), Standard Deviation, Telescopes, X Ray Sources

Scientific paper

A region of the sky close to the COS B source CG 135 + 1 was studied
over the photon energy range 20 keV-25 MeV from balloon altitudes on
1978 October 8. A five-standard-deviation excess was measured in the
counting rate of the telescope above 120 keV, and the spectrum of the
source was evaluated.

Affiliated with

Also associated with

No associations

Rating

Low-energy gamma-ray emission close to CG 135 + 1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low-energy gamma-ray emission close to CG 135 + 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-energy gamma-ray emission close to CG 135 + 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-803510