Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique

Details Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1351z&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1351-1355 (1997).

Computer Science

1

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

Scientific paper

The quasar PKS0528+134 was observed to flare by EGRET/CGRO during the viewing period 213 (VP213). COMPTEL 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.

Affiliated with

Also associated with

No associations

Rating

Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique 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 Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Imaging analysis of PKS0528+134 during its flare with a direct demodulation technique will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-834599