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GRB 200826A

Time: 04:29:52
Trigger Number: Fermi
Burst Advocate:

BAT Data:

RA: a 4.7
00:18:48.0
Dec: a 35.3
35:18:00.0
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 00:27:08.46
Dec: a 34:01:36.6
90% Error Radius: b 2.7
Time to First Observation: c 59900
Early Flux: d n/a
11 Hour Flux: d 0.102190528
24 Hour Flux: d 0.048281189
Initial Temporal Index: -0.9611
Spectral Index (Gamma): 1.54702
Column Density (NH): e 1.199502

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 140000
V Magnitude: n/a
Other Filter Magnitudes: White=21.86

a J2000; b arcsec; c seconds

Other Burst Info:

Redshift:
Host Galaxy:
Other Observatory Detections:

Comments:

Fermi: GCN 28284
UVOT: The UVOT detection is possibly explained by the underlying galaxy emission.

References:

BAT:
XRT: GCN 28300; Evans et al., 2009, MNRAS, 397, 1177
UVOT: GCN 28300
Radio:
Redshift:
Host:
Other: