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![]() 09/11/17 10:15:40 GMT
Palmer et al., GCN 10165; Fermi/GBM trigger #279740477 ; Briggs et al., GCN 10164) triggered the Suzaku Wide-band All-sky Monitor (WAM) which covers an energy range of 50 keV - 5 MeV at 2009-11-12 17:41:16.31 UT (=T0). The observed light curve shows a multi-peaked structure starting at T0-4s, ending at T0+16s with a duration (T90) of about 15 seconds. The fluence in 100-1000 keV was 7.85(-2.91...Full Text
![]() 09/11/13 04:20:04 GMT
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![]() 09/11/13 00:30:38 GMT
"At 17:41:15.82 UT on 12 Nov 2009, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 091112 (trigger 279740477 / 091112.737), which was also detected by the SWIFT-BAT (V. Mangano et al., GCN 10162) The GBM on-ground location is consistent with the Swift position. The angle from the Fermi LAT boresight is 82 degrees. The GBM light curve consists primarily of a broad peak, and has a duration...Full Text
![]() 09/11/12 17:57:24 GMT
At 17:41:21 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 091112 (trigger=375659). Swift could not slew to the burst due to the Sun constraint. The BAT on-board calculated location is RA, Dec 257.728, -36.715 which is RA(J2000) = 17h 10m 55s Dec(J2000) = -36d 42' 53" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The...Full Text Displaying messages 1 to 4
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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