| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB130701060 |
|
| T0 |
1:27:05.761 UTC |
Fermi_GBM |
| ra |
97.7900° |
Fermi_GBM |
| decl |
-60.1300° |
Fermi_GBM |
| pos_error |
3.27e+00° |
Fermi_GBM |
| T90 |
20.224 s |
Fermi_GBM |
| T90_error |
1.729 s |
Fermi_GBM |
| T90_start |
1:27:05.761 UTC |
Fermi_GBM |
| fluence |
7.12e-06 erg/cm² |
Fermi_GBM |
| fluence_error |
9.84e-08 erg/cm² |
Fermi_GBM |
| T100 |
20.224 s |
|
| GBM_located |
True |
|
| mjd |
56474.06048334491 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB130701060 |
| trigger_name |
bn130701060 |
| ra |
97.7900° |
| decl |
-60.1300° |
| pos_error |
3.27e+00° |
| datum |
2013-07-01 |
| t_trigger |
1:27:06.273 UTC |
| T90 |
20.224 s |
| T90_error |
1.729 s |
| T90_start |
1:27:05.761 UTC |
| fluence |
7.12e-06 erg/cm² |
| fluence_error |
9.84e-08 erg/cm² |
| flux_1024 |
1.05e+01 erg/cm²/s |
| flux_1024_error |
4.47e-01 erg/cm²/s |
| flux_1024_time |
3.52e+00 erg/cm²/s |
| flux_64 |
1.26e+01 erg/cm²/s |
| flux_64_error |
2.23e+00 erg/cm²/s |
| GCN 14962 table |
|---|
| GRB_name |
GRB130701B |
| GCN_number |
14962 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
1:27:06.270 UTC |
| ra |
97.8000° |
| decl |
-60.1000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 14962
SUBJECT: GRB 130701B: Fermi GBM detection
DATE: 13/07/01 22:11:12 GMT
FROM: Veronique Pelassa at UAH
V. Pelassa (UAH) reports on behalf of the Fermi GBM Team:
"At 01:27:06.27 UT on July 1st 2013, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 130701B (trigger 394334829 / 130701060).
The on-ground calculated location, using the GBM trigger
data, is RA = 97.8, DEC = -60.1 (J2000 degrees,
equivalent to +06h 31m, -60d 07'), with an uncertainty
of 1.00 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 132 degrees.
The GBM light curve consists of a single pulse
with a duration (T90) of about 20 s (50-300 keV).
The time-averaged spectrum from T0-2.048 s to T0+12.288 s
best fit by a power law function with an exponential
high-energy cutoff. The power law index is -1.04 +/- 0.04 and
the cutoff energy, parameterized as Epeak, is 564 +/- 55 keV
(Castor statistics 599.92 for 492 d.o.f.).
The event fluence (10-1000 keV) in this time interval is
(1.28 +/- 0.03)E-05 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0+3.52 s in the 10-1000 keV band
is 10.5 +/- 0.4 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
|