| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB110301214 |
|
| T0 |
5:08:43.070 UTC |
Fermi_GBM |
| ra |
229.3500° |
Fermi_GBM |
| decl |
29.4000° |
Fermi_GBM |
| pos_error |
2.47e+00° |
Fermi_GBM |
| T90 |
5.693 s |
Fermi_GBM |
| T90_error |
0.362 s |
Fermi_GBM |
| T90_start |
5:08:43.073 UTC |
Fermi_GBM |
| fluence |
3.59e-05 erg/cm² |
Fermi_GBM |
| fluence_error |
3.07e-08 erg/cm² |
Fermi_GBM |
| T100 |
5.696 s |
|
| GBM_located |
True |
|
| mjd |
55621.21438738426 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB110301214 |
| trigger_name |
bn110301214 |
| ra |
229.3500° |
| decl |
29.4000° |
| pos_error |
2.47e+00° |
| datum |
2011-03-01 |
| t_trigger |
5:08:43.070 UTC |
| T90 |
5.693 s |
| T90_error |
0.362 s |
| T90_start |
5:08:43.073 UTC |
| fluence |
3.59e-05 erg/cm² |
| fluence_error |
3.07e-08 erg/cm² |
| flux_1024 |
1.01e+02 erg/cm²/s |
| flux_1024_error |
8.76e-01 erg/cm²/s |
| flux_1024_time |
1.92e+00 erg/cm²/s |
| flux_64 |
1.30e+02 erg/cm²/s |
| flux_64_error |
3.85e+00 erg/cm²/s |
| GCN 11771 table |
|---|
| GRB_name |
GRB110301A |
| GCN_number |
11771 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
5:08:43.070 UTC |
| ra |
229.3500° |
| decl |
29.4000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 11771
SUBJECT: GRB 110301A: Fermi GBM detection
DATE: 11/03/03 08:56:47 GMT
FROM: Suzanne Foley at MPE
S. Foley (MPE)
reports on behalf of the Fermi GBM Team:
"At 05:08:43.07 UT on 01 March 2011, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 110301A (trigger 320648925 / 110301214).
The on-ground calculated location, using the GBM trigger
data, is RA = 229.35, DEC = 29.40 (J2000 degrees,
equivalent to 15 h 17 m 24 s, 29 d 24 ' 00"), with an uncertainty
of 1.0 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 94 degrees.
GBM triggered an automatic repoint request to the Fermi
Observatory to execute a maneuver following this trigger
and track the burst location for the next 5 hours.
However due to Earth-avoidance constraints, the slew did not
commence until ~40 minutes after the trigger.
The GBM light curve consists of a structured single pulse
with a duration (T90) of about 5 s (50-300 keV).
The time-averaged spectrum from T0+0.002 s to T0+5.824 s is
best fit by a Band function with Epeak = 106.80 (+1.85/-1.75) keV,
alpha = -0.81 (+/-0.02), and beta = -2.70 (+0.04/-0.05).
The event fluence (10-1000 keV) in this time interval is
(3.65 +/- 0.03)E-05 erg/cm^2. The 64-ms peak photon flux measured
starting from T0+3.97 s in the 10-1000 keV band
is 125.73 +/- 3.47 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
|