Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB091126389 |
|
T0 |
9:19:48.525 UTC |
Fermi_GBM |
ra |
47.4200° |
Fermi_GBM |
decl |
31.5200° |
Fermi_GBM |
pos_error |
5.04e+00° |
Fermi_GBM |
T90 |
0.024 s |
Fermi_GBM |
T90_error |
0.097 s |
Fermi_GBM |
T90_start |
9:19:48.525 UTC |
Fermi_GBM |
fluence |
1.86e-07 erg/cm² |
Fermi_GBM |
fluence_error |
8.43e-09 erg/cm² |
Fermi_GBM |
T100 |
0.024 s |
|
GBM_located |
True |
|
mjd |
55161.38875607639 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB091126389 |
trigger_name |
bn091126389 |
ra |
47.4200° |
decl |
31.5200° |
pos_error |
5.04e+00° |
datum |
2009-11-26 |
t_trigger |
9:19:48.533 UTC |
T90 |
0.024 s |
T90_error |
0.097 s |
T90_start |
9:19:48.525 UTC |
fluence |
1.86e-07 erg/cm² |
fluence_error |
8.43e-09 erg/cm² |
flux_1024 |
3.27e-01 erg/cm²/s |
flux_1024_error |
1.82e-01 erg/cm²/s |
flux_1024_time |
-6.40e-02 erg/cm²/s |
flux_64 |
4.02e+00 erg/cm²/s |
flux_64_error |
7.82e-01 erg/cm²/s |
GCN 10225 table |
GRB_name |
GRB091126B |
GCN_number |
10225 |
Detection_method |
Fermi GBM Det |
t_trigger |
9:19:48.530 UTC |
ra |
47.4000° |
decl |
31.5000° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 10225
SUBJECT: GRB 091126B: Fermi GBM detection
DATE: 09/12/01 16:57:03 GMT
FROM: Sheila McBreen at MPE
S. McBreen (UCD/MPE) reports on behalf
of the Fermi GBM Team:
"At 09:19:48.53 UT on 26 November 2009, the Fermi Gamma-Ray
Burst Monitor triggered and located a short burst GRB 091126B
(trigger 280919990/091126389).
The on-ground calculated location, using the GBM trigger
data, is RA = 47.4, DEC = 31.5 (J2000 degrees,
equivalent to 03 h 10 m, 31 d 30 '), with an uncertainty
of 14.3 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 60 degrees.
This burst was also independently detected by INTEGRAL SPI-ACS.
The GBM light curve consists of one pulse
with a duration of about 30 ms (8-1000 keV).
The time-averaged spectrum from T0-0.016 s to T0+0.016 s is
adequately fit by a power law function with an exponential
high energy cutoff. The power law index is -0.23 (+0.32/-0.23) and
the cutoff energy, parameterized as Epeak, is 731 (+229/-165) keV
(CSTAT 753 for 846 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(2.2 +/- 0.02)E-07 erg/cm^2. The 16 ms peak photon flux measured
starting from T0-0.008 s in the 8-1000 keV band
is 20.5 +/- 1.3 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
|