| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB090510325 |
|
| T0 |
7:47:38.488 UTC |
Fermi_GBM |
| ra |
269.4000° |
Fermi_GBM |
| decl |
-57.9000° |
Fermi_GBM |
| pos_error |
1.44e+01° |
Fermi_GBM |
| T90 |
7.424 s |
Fermi_GBM |
| T90_error |
1.717 s |
Fermi_GBM |
| T90_start |
7:47:38.488 UTC |
Fermi_GBM |
| fluence |
5.60e-07 erg/cm² |
Fermi_GBM |
| fluence_error |
2.75e-08 erg/cm² |
Fermi_GBM |
| T100 |
7.424 s |
|
| GBM_located |
True |
|
| mjd |
54961.32475101852 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB090510325 |
| trigger_name |
bn090510325 |
| ra |
269.4000° |
| decl |
-57.9000° |
| pos_error |
1.44e+01° |
| datum |
2009-05-10 |
| t_trigger |
7:47:39.512 UTC |
| T90 |
7.424 s |
| T90_error |
1.717 s |
| T90_start |
7:47:38.488 UTC |
| fluence |
5.60e-07 erg/cm² |
| fluence_error |
2.75e-08 erg/cm² |
| flux_1024 |
1.81e+00 erg/cm²/s |
| flux_1024_error |
2.47e-01 erg/cm²/s |
| flux_1024_time |
-3.84e-01 erg/cm²/s |
| flux_64 |
3.14e+00 erg/cm²/s |
| flux_64_error |
1.21e+00 erg/cm²/s |
| GCN 9347 table |
|---|
| GRB_name |
GRB090510B |
| GCN_number |
9347 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
7:47:39.510 UTC |
| ra |
269.4000° |
| decl |
-57.9000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 9347
SUBJECT: GRB 090510B: Fermi GBM detection
DATE: 09/05/11 16:02:42 GMT
FROM: Arne Rau at MPE
Arne Rau (MPE) reports on behalf of the Fermi GBM Team:
"At 07:47:39.51 UT on 10 May 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090510B (trigger 263634461 / 090510325).
The on-ground calculated location, using the GBM trigger
data, is RA = 269.4 , DEC = -57.9 (J2000 degrees,
equivalent to 17h 57m, -57d 56'), with an uncertainty
of 11.6 degrees (radius, 1-sigma containment,
statistical only; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).
The GBM light curve shows a single peak with a duration (T90)
of about 7s (8-1000 keV).
The angle from the Fermi LAT boresight is 100 degrees.
Since the source is weak, the time-averaged spectrum is poorly
constrained."
|