GRB 091117

Time: 17:44:29
Trigger Number: IPN
Burst Advocate: Jay Cummings

BAT Data:

RA: a	30.945 02:03:46.8
Dec: a	-16.944 -16:56:38.4
90% Error Radius: b	2.6
T90: c	0.43
Fluence: d	3.5 (1.2)
1s Peak Photon Flux: e	2.5 (0.5)
Photon Index: f	0.8, PL (0.3)

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90% error in parentheses,
^a J2000; ^b arcmin; ^c seconds; ^d 10^-7 erg/cm² (15-150 keV); ^e ph/cm²/sec (15-150 keV); ^f PL = simple power-law, CPL = cutoff power-law (15-150 keV)

BAT Light Curve:

XRT Data:

RA: a	n/a
Dec: a	n/a
90% Error Radius: b	n/a
Time to First Observation: c	96765
Early Flux: d	n/a
11 Hour Flux: d	n/a
24 Hour Flux: d	n/a
Initial Temporal Index:	n/a
Spectral Index (Gamma):	n/a
Column Density (NH): e	n/a

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Note: Please be aware that only the very basic temporal and spectral quantities are reported here. You are strongly encouraged to see the referenced GCN circulars for full details.
^a J2000; ^b arcsec; ^c seconds; ^d 10^-11 erg/cm²/s (0.3-10 keV); ^e 10²¹ cm^-2

UVOT Data:

RA: a	n/a
Dec: a	n/a
90% Error Radius: b	n/a
Time to First Observation: c	96767
V Magnitude:	n/a
Other Filter Magnitudes:	n/a

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^a J2000; ^b arcsec; ^c seconds

Comments:

Found in ground analysis after the Suzaku WAM alerted the IPN.
The BAT position is inside the error box of a triangulation performed using Konus-Wind, BAT, Suzaku-WAM, and INTEGRAL-SPI-ACS data. A Swift TOO observation has been requested and approved.
XRT: no detection
UVOT: no detection

References:

BAT: GCN 10171; GCN 10180
XRT: GCN 10173; GCN 10177; GCN 10179; GCN 10181; GCN 10292
UVOT: GCN 10184
Radio:
Redshift:
Host:
Other: