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GRB 130807A

Time: 10:25:43
Trigger Number: 565651
Burst Advocate: Andrea Melandri

BAT Data:

RA: a 269.801
17:59:12.2
Dec: a -27.616
-27:36:57.6
90% Error Radius: b 1.7
T90: c n/a
Fluence: d 12 (2)
1s Peak Photon Flux: e 0.4 (0.1)
Photon Index: f 0.31, CPL (0.89)

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:

BAT Light Curve for GRB 130807A

XRT Data:

RA: a 17:59:12.16
Dec: a -27:36:57.5
90% Error Radius: b 3.6
Time to First Observation: c 84.95
Early Flux: d n/a
11 Hour Flux: d 0.0896544
24 Hour Flux: d 0.04383357
Initial Temporal Index: -1.811
Spectral Index (Gamma): 2.30611
Column Density (NH): e 14.6014

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

» XRT GRB Live Catalogue
» XRT Light Curves
» XRT Spectra

UVOT Data:

RA: a n/a
Dec: a n/a
90% Error Radius: b n/a
Time to First Observation: c 145
V Magnitude: V>19.34
Other Filter Magnitudes: B>20.3
U>19.9
UVW1>19.6
UVM2>19.7
UVW2>20.2
White>21.1

a J2000; b arcsec; c seconds

Other Burst Info:

Redshift:
Host Galaxy:
Other Observatory Detections:

Comments:

BAT: The current analysis of the BAT data does not allow us to distinguish between the interpretations of this event as either a GRB or galactic transient.
XRT: It is likely that BAT trigger 565651 was a somewhat unusual GRB rather than a Galactic or extragalactic transient, in spite of its proximity to the Galactic center.
UVOT: no detection

References:

BAT: GCN 15082; GCN 15083
XRT: GCN 15082; GCN 15085; Evans et al., 2009, MNRAS, 397, 1177
UVOT: GCN 15082; GCN 15086
Radio:
Redshift:
Host:
Other: GCN Report 449.1