LogN-LogF distribution of BATSE bursts based on the average flux during high power emission

Details LogN-LogF distribution of BATSE bursts based on the average flux during high power emission LogN-LogF distribution of BATSE bursts based on the average flux during high power emission

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..526...73a&link_type=abstract

GAMMA-RAY BURSTS: 5th Huntsville Symposium. AIP Conference Proceedings, Volume 526, pp. 73-77 (2000).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, Observational Cosmology, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Cosmic Rays

Scientific paper

A physically-based flux characteristic for gamma-ray bursts is proposed that consists of the photon flux in a particular energy range positioned at the peak of the energy spectrum accumulated during the sum of emission time intervals. LogN-LogF distributions are investigated using these fluxes for bright BATSE bursts with peak fluxes on the 64 ms time scale larger than 2 ph/cm2.s. .

Affiliated with

Also associated with

No associations

Rating

LogN-LogF distribution of BATSE bursts based on the average flux during high power emission 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 LogN-LogF distribution of BATSE bursts based on the average flux during high power emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and LogN-LogF distribution of BATSE bursts based on the average flux during high power emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1522203