Compton Telescope Observation of Gamma-Ray Flare from Quasar PKS0528+134

Details Compton Telescope Observation of Gamma-Ray Flare from Quasar PKS0528+134 Compton Telescope Observation of Gamma-Ray Flare from Quasar PKS0528+134

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997chphl..14..395z&link_type=abstract

Chinese Physics Letters, Volume 14, Issue 5, pp. 395-398 (1997).

Physics

Scientific paper

The quasar PKS0528+134 was observed to flare by the energetic gamma-ray experiment (EGRET) γ-ray telescope on the Compton gamma-ray observatory during the viewing period 213 (VP213). The Compton telescope data from VP213 have been reanalyzed by using the direct demodulation method. Images of the source are obtained at energies above 3 MeV and the time variability in the energy range 10-30 MeV is consistent with the result of EGRET. There is no spectral break at energies above 3 MeV during the flare.

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