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