Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors

Details Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..428..466p&link_type=abstract

Fourth Huntsville gamma-ray burst symposium. AIP Conference Proceedings, Volume 428, pp. 466-470 (1998).

Physics

1

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray Sources, X-Ray Bursts, Gamma-Ray, X-Ray, Spectroscopy And Spectrophotometry

Scientific paper

Recent BeppoSAX and RXTE observations have drawn renewed attention to X-ray afterglow from gamma-ray bursts. The low-energy sensitivity of the BATSE Spectroscopy Detectors (SDs) may be exploited to detect GRB afterglow at energies below 20 keV. Application of the Earth occultation technique to SD data allows us to search for 6-20 keV emission on time scales from tens of minutes to many days. We present preliminary results of such a search using a sample of sufficiently well-located BATSE bursts.

Affiliated with

Also associated with

No associations

Rating

Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors 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 Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for X-ray afterglow from GRBs using the BATSE Spectroscopy Detectors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1366639