| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB090304216 |
|
| T0 |
5:10:47.901 UTC |
Fermi_GBM |
| ra |
195.9000° |
Fermi_GBM |
| decl |
-73.4000° |
Fermi_GBM |
| pos_error |
7.96e+00° |
Fermi_GBM |
| T90 |
2.816 s |
Fermi_GBM |
| T90_error |
0.923 s |
Fermi_GBM |
| T90_start |
5:10:47.901 UTC |
Fermi_GBM |
| fluence |
8.99e-07 erg/cm² |
Fermi_GBM |
| fluence_error |
1.02e-07 erg/cm² |
Fermi_GBM |
| T100 |
2.816 s |
|
| GBM_located |
True |
|
| mjd |
54894.2158321875 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB090304216 |
| trigger_name |
bn090304216 |
| ra |
195.9000° |
| decl |
-73.4000° |
| pos_error |
7.96e+00° |
| datum |
2009-03-04 |
| t_trigger |
5:10:48.157 UTC |
| T90 |
2.816 s |
| T90_error |
0.923 s |
| T90_start |
5:10:47.901 UTC |
| fluence |
8.99e-07 erg/cm² |
| fluence_error |
1.02e-07 erg/cm² |
| flux_1024 |
1.91e+00 erg/cm²/s |
| flux_1024_error |
1.58e-01 erg/cm²/s |
| flux_1024_time |
1.28e-01 erg/cm²/s |
| flux_64 |
3.40e+00 erg/cm²/s |
| flux_64_error |
5.24e-01 erg/cm²/s |
| GCN 8930 table |
|---|
| GRB_name |
GRB090304A |
| GCN_number |
8930 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
5:10:48.160 UTC |
| ra |
246.4000° |
| decl |
-80.9000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 8930
SUBJECT: GRB 090304: Fermi GBM detection
DATE: 09/03/04 16:14:43 GMT
FROM: Arne Rau at MPE
Arne Rau (MPE) reports on behalf of the Fermi GBM Team:
"At 05:10:48.16 UT on 04 March 2009, the Fermi Gamma-ray Burst Monitor (GBM)
triggered and located GRB 090304 (trigger 257836250 / 090304.216).
The on-ground calculated location, using the Fermi GBM trigger data,
is RA = 246.4, Dec = -80.9 (J2000 degrees, equivalent to
J2000 16h 25m, -80d 54'), with a statistical uncertainty of 13.1 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 31 degrees.
Since the source is weak, the time-averaged spectrum is poorly constrained.
This event has also been detected by INTEGRAL SPI-ACS."
|