| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB100814351 |
|
| T0 |
8:25:24.978 UTC |
Fermi_GBM |
| ra |
122.8200° |
Fermi_GBM |
| decl |
18.4900° |
Fermi_GBM |
| pos_error |
3.09e+00° |
Fermi_GBM |
| T90 |
7.424 s |
Fermi_GBM |
| T90_error |
0.923 s |
Fermi_GBM |
| T90_start |
8:25:24.978 UTC |
Fermi_GBM |
| fluence |
4.15e-06 erg/cm² |
Fermi_GBM |
| fluence_error |
4.08e-08 erg/cm² |
Fermi_GBM |
| T100 |
7.424 s |
|
| GBM_located |
True |
|
| mjd |
55422.35098354167 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB100814351 |
| trigger_name |
bn100814351 |
| ra |
122.8200° |
| decl |
18.4900° |
| pos_error |
3.09e+00° |
| datum |
2010-08-14 |
| t_trigger |
8:25:25.746 UTC |
| T90 |
7.424 s |
| T90_error |
0.923 s |
| T90_start |
8:25:24.978 UTC |
| fluence |
4.15e-06 erg/cm² |
| fluence_error |
4.08e-08 erg/cm² |
| flux_1024 |
1.04e+01 erg/cm²/s |
| flux_1024_error |
3.66e-01 erg/cm²/s |
| flux_1024_time |
3.58e+00 erg/cm²/s |
| flux_64 |
1.32e+01 erg/cm²/s |
| flux_64_error |
1.56e+00 erg/cm²/s |
| GCN 11130 table |
|---|
| GRB_name |
GRB100814B |
| GCN_number |
11130 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
8:25:25.750 UTC |
| ra |
122.8000° |
| decl |
18.5000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 11130
SUBJECT: GRB 100814B: Fermi GBM detection
DATE: 10/08/19 16:13:07 GMT
FROM: Andreas von Kienlin at MPE
A. von Kienlin (MPE) reports on behalf of the Fermi GBM Team:
"The Fermi Gamma-ray Burst Monitor (GBM) trigger 303467127 / 100814351
at 08:25:25.75 UT on 14 August 2010, tentatively classified as a
solar flare, is in fact due to a GRB.
The on-ground calculated location of GRB 100814B , using the
GBM trigger data, is RA = 122.8, DEC = +18.5 (J2000 degrees,
equivalent to 08h 11m, +18d 30'), with an uncertainty
of 2.6 degrees (radius, 1-sigma containment,
statistical only; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).
The angle from the Fermi LAT boresight is 87 degrees.
The GBM light curve consists of a single pulse
with a duration (T90) of about 6.4 +/- 1.1 s (50-300 keV).
The time-averaged spectrum from T0-3.072 s to T0+9.216 s is
best fit by a Band function with Epeak = 81.0 +6.2/-6.7 keV,
alpha = -0.62 +0.14/-0.11, and beta = -2.49 +0.15/-0.20
(Castor C-STAT 521 for 488 d.o.f.).
The event fluence (10-1000 keV) in this time interval is
(4.7 +/- 0.2)E-06 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0+3.584 s in the 10-1000 keV band
is 10.4 +/- 0.3 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
|