| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB201011629 |
|
| T0 |
15:06:22.867 UTC |
Fermi_GBM |
| ra |
281.0500° |
Fermi_GBM |
| decl |
-5.7200° |
Fermi_GBM |
| pos_error |
4.84e+00° |
Fermi_GBM |
| T90 |
126.21 s |
Fermi_GBM |
| T90_error |
1.493 s |
Fermi_GBM |
| T90_start |
15:06:22.867 UTC |
Fermi_GBM |
| fluence |
7.49e-06 erg/cm² |
Fermi_GBM |
| fluence_error |
4.48e-08 erg/cm² |
Fermi_GBM |
| T100 |
126.21 s |
|
| GBM_located |
True |
|
| mjd |
59133.62943133102 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB201011629 |
| trigger_name |
bn201011629 |
| ra |
281.0500° |
| decl |
-5.7200° |
| pos_error |
4.84e+00° |
| datum |
2020-10-11 |
| t_trigger |
15:06:24.659 UTC |
| T90 |
126.21 s |
| T90_error |
1.493 s |
| T90_start |
15:06:22.867 UTC |
| fluence |
7.49e-06 erg/cm² |
| fluence_error |
4.48e-08 erg/cm² |
| flux_1024 |
5.82e+00 erg/cm²/s |
| flux_1024_error |
2.86e-01 erg/cm²/s |
| flux_1024_time |
5.44e+00 erg/cm²/s |
| flux_64 |
1.18e+01 erg/cm²/s |
| flux_64_error |
1.29e+00 erg/cm²/s |
| GCN 28606 table |
|---|
| GRB_name |
GRB201011A |
| GCN_number |
28606 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
15:06:24.660 UTC |
| ra |
281.1000° |
| decl |
-5.7000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 28606
SUBJECT: GRB 201011A: Fermi GBM detection of a likely Long GRB in the direction of SGR 1830-0645
DATE: 20/10/12 21:10:54 GMT
FROM: Oliver J Roberts at USRA/NASA
O.J. Roberts (USRA) and C. Meegan (UAH)
report on behalf of the Fermi GBM Team:
"At 15:06:24.66 UT on 11 October 2020, the Fermi Gamma-Ray Burst Monitor (GBM)
triggered and located GRB 201011A (trigger 624121589 / 201011629),
which was also detected by the AGILE (Ursi et al. 2020, GCN 28605).
The on-ground calculated location, using the Fermi GBM trigger data,
is RA = 281.1, Dec = -5.7 (J2000 degrees, equivalent to
J2000 18h 44m , -05d 43'), with a statistical uncertainty of 2.4 degrees.
The angle from the Fermi LAT boresight at the GBM trigger time is 35 degrees.
The GBM light curve consists of multiple pulses
with a duration (T90) of about 126.2 s (50-300 keV).
The time-averaged spectrum from T0-1.8 s to T0+124.2 s is
best fit by a power law function with an exponential
high-energy cutoff. The power law index is -1.18 (+0.09/-0.08) and
the cutoff energy, parameterized as Epeak, is 138.0 (+19.6/-14.4) keV.
The event fluence (10-1000 keV) in this time interval is
(9.25 +/- 0.52)E-06 erg/cm^2. The 1s peak photon flux measured
starting from T0+5.44 s in the 10-1000 keV band
is 5.8 +/- 0.3 ph/s/cm^2.
We note that this event is in the direction of SGR 1830-0645
(K.L. Page et al. 2020, GCN 28594). While we cannot conclusively rule out
an association with SGR 1830-0645, the GBM spectrum and time history
are suggestive of a long GRB and not a Magnetar transient.
Analysis is ongoing to confirm the source.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog:
https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html
For Fermi GBM data and info, please visit the official Fermi GBM Support Page:
https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/"
|