| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB090403314 |
|
| T0 |
7:32:39.826 UTC |
Fermi_GBM |
| ra |
67.1000° |
Fermi_GBM |
| decl |
47.2000° |
Fermi_GBM |
| pos_error |
6.09e+00° |
Fermi_GBM |
| T90 |
14.848 s |
Fermi_GBM |
| T90_error |
1.846 s |
Fermi_GBM |
| T90_start |
7:32:39.826 UTC |
Fermi_GBM |
| fluence |
1.09e-06 erg/cm² |
Fermi_GBM |
| fluence_error |
1.93e-08 erg/cm² |
Fermi_GBM |
| T100 |
14.848 s |
|
| GBM_located |
True |
|
| mjd |
54924.314349837965 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB090403314 |
| trigger_name |
bn090403314 |
| ra |
67.1000° |
| decl |
47.2000° |
| pos_error |
6.09e+00° |
| datum |
2009-04-03 |
| t_trigger |
7:32:42.130 UTC |
| T90 |
14.848 s |
| T90_error |
1.846 s |
| T90_start |
7:32:39.826 UTC |
| fluence |
1.09e-06 erg/cm² |
| fluence_error |
1.93e-08 erg/cm² |
| flux_1024 |
1.82e+00 erg/cm²/s |
| flux_1024_error |
2.07e-01 erg/cm²/s |
| flux_1024_time |
-5.76e-01 erg/cm²/s |
| flux_64 |
3.02e+00 erg/cm²/s |
| flux_64_error |
1.08e+00 erg/cm²/s |
| GCN 9097 table |
|---|
| GRB_name |
GRB090403A |
| GCN_number |
9097 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
7:32:42.130 UTC |
| ra |
65.2000° |
| decl |
47.1000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 9097
SUBJECT: GRB 090403: Fermi GBM detection
DATE: 09/04/06 15:22:07 GMT
FROM: Sheila McBreen at MPE
Sheila McBreen (UCD/MPE) reports on behalf of the Fermi GBM Team:
"At 07:32:42.13 UT on 03 April 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090403 (trigger 260436764 / 090403314).
The on-ground calculated location, using the GBM trigger
data, is RA = 65.2, DEC = +47.1 (J2000 degrees,
equivalent to 04 h 21 m, +47 d 06'), with an uncertainty
of 8.5 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 42 degrees.
The GBM light curve consists of one pulse
with a duration of about 16 s. Since the source is weak,
the time-averaged spectrum is poorly constrained."
|