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GRB 260915A

Time: 01:12:03
Trigger Number: SVOM
Burst Advocate:

BAT Data:

RA: a 8.1021
00:32:24.5
Dec: a 8.2587
08:15:31.3
90% Error Radius: b n/a
T90: c n/a
Fluence: d n/a (n/a)
1s Peak Photon Flux: e n/a (n/a)
Photon Index: f n/a (n/a)

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)

XRT Data:

RA: a 00:32:37.11
Dec: a 08:14:55.5
90% Error Radius: b 8.5
Time to First Observation: c 174400
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): 1.945608672
Column Density (NH): e 0.42536750203156

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 n/a
V Magnitude: n/a
Other Filter Magnitudes: n/a

a J2000; b arcsec; c seconds

Other Burst Info:

Redshift:
Host Galaxy:
Other Observatory Detections:

Comments:

SVOM: GCN 45570
XRT: While the source does not fade during the Swift-XRT observation, the measured flux is more than an order of magnitude below the EP value reported in GCN 45587. This source is therefore believed to be the afterglow.

References:

BAT:
XRT: GCN 45623; Evans et al., 2009, MNRAS, 397, 1177
UVOT:
Radio:
Redshift:
Host:
Other: