Other
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..152r&link_type=abstract
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 152-155 (2010).
Other
Gamma-Ray Sources (Astronomical), X-Ray Spectra, Brightness, Redshift, Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray, Luminosity And Mass Functions, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies
Scientific paper
The small population of Fermi LAT detected GRBs discovered over the last two years has been providing interesting and unexpected clues into GRB prompt and afterglow emission mechanisms. Over the last 5 years, it has been Swift that has provided the robust data set of UV/optical and X-ray afterglow observations that opened many windows into other components of GRB emission structure. We explore the new ability to utilize both of these observatories to study the same GRBs over 10 orders of magnitude in energy, although not always concurrently. Almost all LAT GRBs that have been followed-up by Swift within 1-day have been clearly detected and carefully observed. We will present the context of the lower-energy afterglows of this special subset of GRBs that has >100 MeV emission compared to the hundreds in the Swift database that may or may not have been observed by LAT, and theorize upon the relationship between these properties and the origin of the high energy gamma-ray emission.
No associations
LandOfFree
Afterglow Populations Studies from Swift Follow-up of Fermi-LAT GRBs 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 Afterglow Populations Studies from Swift Follow-up of Fermi-LAT GRBs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Afterglow Populations Studies from Swift Follow-up of Fermi-LAT GRBs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1402936