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![]() TITLE: GCN CIRCULAR NUMBER: 8781 SUBJECT: GRB 081231: Fermi GBM Detection DATE: 09/01/06 02:43:13 GMT FROM: Adam Goldstein at Fermi-GBM/UAH <adam.m.goldstein@msfc.nasa.gov> A. Goldstein (UAH), and R. Preece (UAH) report on behalf of the Fermi GBM Team: "At 03:21:01.93 UT on 31 December 2008, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 081231 (trigger 252386462 / 081231140). The on-ground calculated location, using the GBM trigger data, is RA = 218.74, DEC = -38.72 (J2000 degrees, equivalent to 14 h 35 m, -38 d 43'), with an uncertainty of 1.0 degree (radius, 1-sigma containment, statistical only; there is additionally a systematic error which is currently estimated to be 2 to 3 degrees). The angle from the Fermi LAT boresight is 20 degrees. This burst was also independently detected by INTEGRAL SPI-ACS. The GBM light curve consists of three main emission peaks with apparent substructure and a duration (T90) of about 29 s (8-1000 keV). The time-averaged spectrum from T0-4.1 s to T0+37.9 s is best fit by a Band function with Epeak = 152.3 +/- 11.9 keV, alpha = -0.80 +/- 0.06, and beta = -2.03 +/- 0.07. (chi squared 998 for 726 d.o.f.). The event fluence (8-1000 keV) in this time interval is 1.2E-05 +/- 5.9E-07 erg/cm^2. The peak photon flux measured starting from T0-4.1 s in the 8-1000 keV band is 1.53 +/- 0.08 ph/s/cm^2. The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog." GRB Position Observations
GRB Observations
This site was created by Robert Quimby
Database maintained by Robert Quimby, Erin McMahon, and Jeremy Murphy Information displayed on this site is compiled from GCN Circulars and other sources as indicated. |
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