| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB100916779 |
|
| T0 |
18:41:12.237 UTC |
Fermi_GBM |
| ra |
151.9600° |
Fermi_GBM |
| decl |
-59.3800° |
Fermi_GBM |
| pos_error |
3.66e+00° |
Fermi_GBM |
| T90 |
12.8 s |
Fermi_GBM |
| T90_error |
2.111 s |
Fermi_GBM |
| T90_start |
18:41:12.237 UTC |
Fermi_GBM |
| fluence |
1.78e-06 erg/cm² |
Fermi_GBM |
| fluence_error |
1.38e-07 erg/cm² |
Fermi_GBM |
| T100 |
12.8 s |
|
| GBM_located |
True |
|
| mjd |
55455.77861385416 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB100916779 |
| trigger_name |
bn100916779 |
| ra |
151.9600° |
| decl |
-59.3800° |
| pos_error |
3.66e+00° |
| datum |
2010-09-16 |
| t_trigger |
18:41:12.493 UTC |
| T90 |
12.8 s |
| T90_error |
2.111 s |
| T90_start |
18:41:12.237 UTC |
| fluence |
1.78e-06 erg/cm² |
| fluence_error |
1.38e-07 erg/cm² |
| flux_1024 |
4.97e+00 erg/cm²/s |
| flux_1024_error |
4.57e-01 erg/cm²/s |
| flux_1024_time |
-2.56e-01 erg/cm²/s |
| flux_64 |
2.13e+01 erg/cm²/s |
| flux_64_error |
2.97e+00 erg/cm²/s |
| GCN 11290 table |
|---|
| GRB_name |
GRB100916A |
| GCN_number |
11290 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
18:41:12.490 UTC |
| ra |
152.0000° |
| decl |
-59.4000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 11290
SUBJECT: GRB 100916A: Fermi GBM detection
DATE: 10/09/18 04:35:26 GMT
FROM: Alexander van der Horst at NASA/MSFC
A.J. van der Horst (NASA/MSFC/ORAU) reports on behalf of the Fermi GBM
Team:
"The Fermi Gamma-Ray Burst Monitor (GBM) trigger 306355274 at
18:41:12.49 UT
on 16 September 2010, tentatively classified as Distant Particles, is in
fact
a GRB. The source location is close to the Earth's limb, which gave rise to
the original classification. The GBM light curve consists of a ~0.5 s short
spike on top of lower level emission extending for ~20 s.
The on-ground location of GRB 100916A, using the GBM trigger data, is
RA = 152.0, Dec = -59.4 (J2000 degrees, equivalent to 10h 08m, -59d 23'),
with an uncertainty of 3.5 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 142
degrees."
|