| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB081206604 |
|
| T0 |
14:29:28.645 UTC |
Fermi_GBM |
| ra |
353.3000° |
Fermi_GBM |
| decl |
-31.9000° |
Fermi_GBM |
| pos_error |
9.14e+00° |
Fermi_GBM |
| T90 |
7.936 s |
Fermi_GBM |
| T90_error |
4.382 s |
Fermi_GBM |
| T90_start |
14:29:28.645 UTC |
Fermi_GBM |
| fluence |
5.00e-07 erg/cm² |
Fermi_GBM |
| fluence_error |
3.66e-08 erg/cm² |
Fermi_GBM |
| T100 |
7.936 s |
|
| GBM_located |
True |
|
| mjd |
54806.60380376157 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB081206604 |
| trigger_name |
bn081206604 |
| ra |
353.3000° |
| decl |
-31.9000° |
| pos_error |
9.14e+00° |
| datum |
2008-12-06 |
| t_trigger |
14:29:30.693 UTC |
| T90 |
7.936 s |
| T90_error |
4.382 s |
| T90_start |
14:29:28.645 UTC |
| fluence |
5.00e-07 erg/cm² |
| fluence_error |
3.66e-08 erg/cm² |
| flux_1024 |
1.90e+00 erg/cm²/s |
| flux_1024_error |
2.09e-01 erg/cm²/s |
| flux_1024_time |
-5.76e-01 erg/cm²/s |
| flux_64 |
3.02e+00 erg/cm²/s |
| flux_64_error |
1.06e+00 erg/cm²/s |
| GCN 8641 table |
|---|
| GRB_name |
GRB081206B |
| GCN_number |
8641 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
14:29:30.690 UTC |
| ra |
346.2000° |
| decl |
-33.1000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 8641
SUBJECT: GRB 081206B: Fermi GBM detection
DATE: 08/12/08 16:52:41 GMT
FROM: Andreas von Kienlin at MPE
A. von Kienlin (MPE)
reports on behalf of the Fermi GBM Team:
"At 14:29:30.69 UT on 06 December 2008, the Fermi Gamma-ray Burst Monitor
(GBM) triggered and located GRB 081206B (trigger 250266571 / 081206604).
The on-ground calculated location, using the Fermi GBM trigger data,
is RA = 346.2, Dec = -33.1 (J2000 degrees, equivalent to
J2000 23h 05m, -33d 06'), with a statistical uncertainty of 13.2 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 82 degrees.
The GBM light curve shows a single peak with a duration of about 10 s. Since
the source is weak, the time-averaged spectrum is poorly constrained."
|