| Summary table |
|---|
| Variable |
Value |
Source |
| GRB_name_Fermi |
GRB140624423 |
|
| T0 |
10:08:40.815 UTC |
Fermi_GBM |
| ra |
23.1600° |
Fermi_GBM |
| decl |
-0.5600° |
Fermi_GBM |
| pos_error |
5.01e+00° |
Fermi_GBM |
| T90 |
0.096 s |
Fermi_GBM |
| T90_error |
0.093 s |
Fermi_GBM |
| T90_start |
10:08:40.815 UTC |
Fermi_GBM |
| fluence |
2.42e-07 erg/cm² |
Fermi_GBM |
| fluence_error |
9.53e-09 erg/cm² |
Fermi_GBM |
| T100 |
0.096 s |
|
| GBM_located |
True |
|
| mjd |
56832.42269461806 |
Fermi_GBM |
| Fermi GBM table |
|---|
| GRB_name_Fermi |
GRB140624423 |
| trigger_name |
bn140624423 |
| ra |
23.1600° |
| decl |
-0.5600° |
| pos_error |
5.01e+00° |
| datum |
2014-06-24 |
| t_trigger |
10:08:40.895 UTC |
| T90 |
0.096 s |
| T90_error |
0.093 s |
| T90_start |
10:08:40.815 UTC |
| fluence |
2.42e-07 erg/cm² |
| fluence_error |
9.53e-09 erg/cm² |
| flux_1024 |
1.52e+00 erg/cm²/s |
| flux_1024_error |
1.70e-01 erg/cm²/s |
| flux_1024_time |
-1.28e-01 erg/cm²/s |
| flux_64 |
1.92e+01 erg/cm²/s |
| flux_64_error |
1.29e+00 erg/cm²/s |
| GCN 16452 table |
|---|
| GRB_name |
GRB140624A |
| GCN_number |
16452 |
| Detection_method |
Fermi GBM Det |
| t_trigger |
10:08:40.900 UTC |
| ra |
23.1600° |
| decl |
-0.5600° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 16452
SUBJECT: GRB 140624A: Fermi GBM observation of a short burst
DATE: 14/06/24 19:23:39 GMT
FROM: George A. Younes at USRA/NASA/MSFC
G. Younes (USRA/NASA-MSFC), A. von Kienlin (MPE), and C. Meegan (UAH)
report on behalf of the Fermi GBM Team:
"At 10:08:40.90 UT on 24 June 2014, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 140624A (trigger 425297323/140624423).
The trigger resulted in an Autonomous Repoint Request (ARR) that was
accepted and the spacecraft slewed to the GBM in-flight location.
The on-ground calculated location, using the GBM trigger
data, is RA = 23.16, DEC = -0.56 (J2000 degrees,
equivalent to 01h 32m, -00d 33'), with an uncertainty
of 4.6 degrees (radius, 1-sigma containment,
statistical only; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).
The angle from the Fermi LAT boresight, using the GBM on-ground
calculated location, is 54 degrees.
The GBM light curve consists of a single peak
with a duration of about 0.1 s (50-300 keV).
The time-averaged spectrum from T0-0.064 s to T0+0.064 s is
adequately fit by a Comptonized function with Epeak = 365 +/- 81 keV,
and alpha = -0.8 +/- 0.1.
The event fluence (10-1000 keV) in this time interval is
(3.0 +/- 0.3)E-07 erg/cm^2. The 0.064 second peak photon flux
measured starting from T0+0.0 s in the 10-1000 keV band
is 19.2 +/- 1.3 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
|