Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB081206987 |
|
T0 |
23:41:44.581 UTC |
Fermi_GBM |
ra |
54.3000° |
Fermi_GBM |
decl |
-8.6000° |
Fermi_GBM |
pos_error |
6.93e+00° |
Fermi_GBM |
T90 |
22.528 s |
Fermi_GBM |
T90_error |
2.919 s |
Fermi_GBM |
T90_start |
23:41:44.581 UTC |
Fermi_GBM |
fluence |
1.13e-06 erg/cm² |
Fermi_GBM |
fluence_error |
3.49e-08 erg/cm² |
Fermi_GBM |
T100 |
22.528 s |
|
GBM_located |
True |
|
mjd |
54806.98732153935 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB081206987 |
trigger_name |
bn081206987 |
ra |
54.3000° |
decl |
-8.6000° |
pos_error |
6.93e+00° |
datum |
2008-12-06 |
t_trigger |
23:41:50.469 UTC |
T90 |
22.528 s |
T90_error |
2.919 s |
T90_start |
23:41:44.581 UTC |
fluence |
1.13e-06 erg/cm² |
fluence_error |
3.49e-08 erg/cm² |
flux_1024 |
1.66e+00 erg/cm²/s |
flux_1024_error |
1.92e-01 erg/cm²/s |
flux_1024_time |
-7.04e-01 erg/cm²/s |
flux_64 |
2.91e+00 erg/cm²/s |
flux_64_error |
9.34e-01 erg/cm²/s |
GCN 8644 table |
GRB_name |
GRB081206C |
GCN_number |
8644 |
Detection_method |
Fermi GBM Det |
t_trigger |
23:41:50.470 UTC |
ra |
41.1200° |
decl |
-14.4200° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 8644
SUBJECT: GRB 081206C: Fermi GBM detection
DATE: 08/12/09 21:03:11 GMT
FROM: Sylvain Guiriec at UAH
S. Guiriec (UAH) and A.J. van der Horst (NASA/MSFC/ORAU)
report on behalf of the Fermi GBM Team:
"At 23:41:50.47 UT on 6 December 2008, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 081206C (trigger 250299711 / 081206987).
The on-ground calculated location, using the GBM trigger data, is
RA = 41.12, DEC = -14.42 (J2000 degrees, equivalent to +2h44m, -14d25'),
with an uncertainty of 7.7 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 71 degrees.
The GBM light curve shows a main pulse of ~20 seconds starting at ~T0-11s.
There is additional weak emission up to T0+83s.
The time-averaged spectrum from T0-9s to T0+11s is adequately fit by a
simple power-law function with index -1.35 +/- 0.04
(chi squared 505 for 481 d.o.f.).
The fluence (50-300 keV) in this time interval is
(1.19 +/- 0.04)E-6 erg/cm^2.
The 1-sec peak photon flux measured starting from T0-1s in the 50-300 keV
band is 0.76 +/- 0.04 ph/s-cm^2.
The spectral and timing analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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