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: