Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231..187d&link_type=abstract
Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 187-190
Astronomy and Astrophysics
Astrophysics
70
Gev: Gamma-Ray Bursts
Scientific paper
EGRET on the Compton Gamma Ray Observatory has detected 5 gammaray bursts above 30 MeV. The sub-MeV emission, as detected by BATSE, for these 5 bursts has the largest fluence,F, and peak intensity,I, of any of the BATSE detected bursts within the EGRET field of view. The BATSE data reported in the 2B catalog and the EGRET exposure,E, are combined to select additional bursts with largeF ×E andI ×E. The EGRET data for these bright BATSE bursts are searched for prompt, as well as delayed, emission above 30 MeV. The average properties of the >30 MeV emission are obtained by adding the EGRET data from the 5 bursts. On average the fluence is greater than 15% of the fluence detected by BATSE below an MeV, and the average spectrum is flatter than the spectrum from 1-30 MeV.
No associations
LandOfFree
EGRET Observations of > 30 MeV Emission from the Brightest Bursts Detected by BATSE 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 EGRET Observations of > 30 MeV Emission from the Brightest Bursts Detected by BATSE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EGRET Observations of > 30 MeV Emission from the Brightest Bursts Detected by BATSE will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-823509