Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB130604033 |
|
T0 |
0:48:11.066 UTC |
Fermi_GBM |
ra |
292.1800° |
Fermi_GBM |
decl |
-24.8600° |
Fermi_GBM |
pos_error |
3.11e+00° |
Fermi_GBM |
T90 |
26.88 s |
Fermi_GBM |
T90_error |
0.923 s |
Fermi_GBM |
T90_start |
0:48:11.066 UTC |
Fermi_GBM |
fluence |
1.75e-05 erg/cm² |
Fermi_GBM |
fluence_error |
1.31e-07 erg/cm² |
Fermi_GBM |
T100 |
26.88 s |
|
GBM_located |
True |
|
mjd |
56447.03346141204 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB130604033 |
trigger_name |
bn130604033 |
ra |
292.1800° |
decl |
-24.8600° |
pos_error |
3.11e+00° |
datum |
2013-06-04 |
t_trigger |
0:48:11.322 UTC |
T90 |
26.88 s |
T90_error |
0.923 s |
T90_start |
0:48:11.066 UTC |
fluence |
1.75e-05 erg/cm² |
fluence_error |
1.31e-07 erg/cm² |
flux_1024 |
1.32e+01 erg/cm²/s |
flux_1024_error |
3.67e-01 erg/cm²/s |
flux_1024_time |
1.57e+01 erg/cm²/s |
flux_64 |
2.00e+01 erg/cm²/s |
flux_64_error |
1.66e+00 erg/cm²/s |
GCN 14765 table |
GRB_name |
GRB130604B |
GCN_number |
14765 |
Detection_method |
Fermi GBM Det |
t_trigger |
0:48:11.320 UTC |
ra |
292.1800° |
decl |
-24.8600° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 14765
SUBJECT: GRB 130604B: Fermi GBM detection
DATE: 13/06/04 18:03:38 GMT
FROM: Andrew Collazzi at NASA/MSFC/ORAU
Andrew C. Collazzi (NASA/ORAU)
reports on behalf of the Fermi GBM Team:
"At 00:48:11.32 UT on 4 June 2013, the Fermi Gamma-ray
Burst Monitor (GBM) triggered and located GRB 130604B
(trigger 391999694 / 130604.033). The on-ground calculated
location, using the Fermi GBM trigger data, is RA = 292.18,
Dec = -24.86 (J2000 degrees, equivalent to J2000
19h 28m, -24d 51'), with a statistical uncertainty of 1.2 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 93 degrees.
The GBM light curve shows a multi-peak burst with a duration (T90)
of about 27 s (50 - 300 keV). The time-averaged
spectrum from T0-8.192 to T0+35.841 s is well fit by a Comptonized
spectrum with Epeak = 227.6 +/- 19.0 and alpha = -1.24 +/- 0.03.
The fluence (10-1000 keV) in this time interval is
(1.79 +/- 0.06)E-05 erg/cm^2. The burst has a 1.024-s peak flux
(10-1000 keV) of 13.24 +/- 0.37 ph/cm^2/s that starts at
T+15.744 s.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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