Very high energy gamma ray extension of GRO observations

Details Very high energy gamma ray extension of GRO observations Very high energy gamma ray extension of GRO observations

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sao..rept.....w&link_type=abstract

Semiannual Status Report No. 3, 1 Jul. - 31 Dec. 1991 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astronomy

Gamma Ray Astronomy, Gamma Ray Observatory, Gamma Ray Telescopes, Spaceborne Telescopes, Gamma Ray Bursts, Gamma Rays

Scientific paper

This has been an exiciting year for high energy gamma-ray astronomy, both from space and from ground-based observatories. It has been a particularly active period for the Whipple Observatory gamma-ray group. In phase 1 of the Compton Gamma Ray Observatory (GRO), there has not been too much opportunity for overlapping observations with the Energetic Gamma Ray Experiment Telescope (EGRET) and the other GRO telescopes; however, significant progress was made in the development of data analysis techniques and in improving the sensitivity of the technique which will have direct application in correlative observations in phase 2. Progress made during the period 1 Jul. 1991 - 31 Dec. 1991 is presented.

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