BATSE Observations of GRB 991216

Details BATSE Observations of GRB 991216 BATSE Observations of GRB 991216

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.3404c&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #34.04; Bulletin of the American Astronomical Society, Vol. 32, p.1244

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations of the afterglow of gamma-ray burst GRB 991216 have been reported at wavelengths from radio to the X-ray band. BATSE observations at energies above 20 keV show intense prompt emission lasting about 40 s followed by a long tail which persists at least 1000 s beyond that time. We present temporal and spectral characteristics of both the prompt and extended emission, and explore whether the tail might be the gamma-ray signature of the afterglow.

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