Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB100130777 |
|
T0 |
18:38:25.223 UTC |
Fermi_GBM |
ra |
78.5700° |
Fermi_GBM |
decl |
20.8300° |
Fermi_GBM |
pos_error |
3.29e+00° |
Fermi_GBM |
T90 |
86.018 s |
Fermi_GBM |
T90_error |
6.988 s |
Fermi_GBM |
T90_start |
18:38:25.223 UTC |
Fermi_GBM |
fluence |
1.39e-05 erg/cm² |
Fermi_GBM |
fluence_error |
1.71e-07 erg/cm² |
Fermi_GBM |
T100 |
86.018 s |
|
GBM_located |
True |
|
mjd |
55226.77668082176 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB100130777 |
trigger_name |
bn100130777 |
ra |
78.5700° |
decl |
20.8300° |
pos_error |
3.29e+00° |
datum |
2010-01-30 |
t_trigger |
18:38:35.463 UTC |
T90 |
86.018 s |
T90_error |
6.988 s |
T90_start |
18:38:25.223 UTC |
fluence |
1.39e-05 erg/cm² |
fluence_error |
1.71e-07 erg/cm² |
flux_1024 |
3.50e+00 erg/cm²/s |
flux_1024_error |
2.00e-01 erg/cm²/s |
flux_1024_time |
2.48e+01 erg/cm²/s |
flux_64 |
5.73e+00 erg/cm²/s |
flux_64_error |
8.81e-01 erg/cm²/s |
GCN 10373 table |
GRB_name |
GRB100130B |
GCN_number |
10373 |
Detection_method |
Fermi GBM Det |
t_trigger |
18:38:35.460 UTC |
ra |
77.6300° |
decl |
20.3600° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 10373
SUBJECT: GRB 100130B: Fermi GBM detection
DATE: 10/02/05 19:33:39 GMT
FROM: Sylvain Guiriec at UAH
Sylvain Guiriec (UAH)
reports on behalf of the Fermi GBM Team:
"At 18:38:35.46 UT on 10 January 2010, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 100130B (trigger 286569517 / 100130777).
The on-ground calculated location, using the GBM trigger
data, is RA = 77.63, DEC = +20.36 (J2000 degrees,
equivalent to 05h10m, +20d21'), with an uncertainty
of 1.41 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 89 degrees.
The GBM light curve consists of 4 peaks
with a duration (T90) of about 90+/-6 s (8-1000 keV).
The time-averaged spectrum from T0-14 s to T0+89 s is
adequately fit by a power law function with an exponential
high energy cutoff. The power law index is -1.22 +/- 0.04 and
the cutoff energy, parameterized as Epeak, is 208.00 +/- 17.10 keV
(Castor C-stat 1074 for 483 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(1.342 +/- 0.047)E-5 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+23.55 s in the 8-1000 keV band
is 3.72 +/- 0.26 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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