EGRET observations of PKS 0528+134 from 1991 to 1997

Details EGRET observations of PKS 0528+134 from 1991 to 1997 EGRET observations of PKS 0528+134 from 1991 to 1997

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1346m&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1346-1350 (1997).

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Quasars, Gamma-Ray, Magnitudes And Colors, Luminosities, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The compact, radio-loud quasar PKS 0528+134 has been one of the brightest active galactic nuclei (AGN) detected by EGRET. The flux history of the source including data up to March 1997, as well as the spectra measured during the flaring and non-flaring states is presented. Multiwavelength observations of PKS 0528+134 are also presented. A detailed relativistic SSC jet model agrees well with the multiwavelength spectrum; the data, however are insufficient to discriminate between this and other emission models.

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