Summary table |
Variable |
Value |
Source |
GRB_name_Fermi |
GRB090514006 |
|
T0 |
0:08:39.157 UTC |
Fermi_GBM |
ra |
12.3000° |
Fermi_GBM |
decl |
-10.9000° |
Fermi_GBM |
pos_error |
3.33e+00° |
Fermi_GBM |
T90 |
43.521 s |
Fermi_GBM |
T90_error |
1.739 s |
Fermi_GBM |
T90_start |
0:08:39.285 UTC |
Fermi_GBM |
fluence |
6.46e-06 erg/cm² |
Fermi_GBM |
fluence_error |
1.07e-07 erg/cm² |
Fermi_GBM |
T100 |
43.649 s |
|
GBM_located |
True |
|
mjd |
54965.00600876157 |
Fermi_GBM |
Fermi GBM table |
GRB_name_Fermi |
GRB090514006 |
trigger_name |
bn090514006 |
ra |
12.3000° |
decl |
-10.9000° |
pos_error |
3.33e+00° |
datum |
2009-05-14 |
t_trigger |
0:08:39.157 UTC |
T90 |
43.521 s |
T90_error |
1.739 s |
T90_start |
0:08:39.285 UTC |
fluence |
6.46e-06 erg/cm² |
fluence_error |
1.07e-07 erg/cm² |
flux_1024 |
6.01e+00 erg/cm²/s |
flux_1024_error |
2.01e-01 erg/cm²/s |
flux_1024_time |
7.04e-01 erg/cm²/s |
flux_64 |
7.80e+00 erg/cm²/s |
flux_64_error |
8.04e-01 erg/cm²/s |
GCN 9398 table |
GRB_name |
GRB090514A |
GCN_number |
9398 |
Detection_method |
Fermi GBM Det |
t_trigger |
0:08:39.160 UTC |
ra |
12.3000° |
decl |
-10.9000° |
Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 9398
SUBJECT: GRB 090514: Fermi GBM detection
DATE: 09/05/19 13:59:08 GMT
FROM: Colleen A. Wilson at NASA/MSFC/NSSTC
Colleen A. Wilson-Hodge (NASA/MSFC)
reports on behalf of the Fermi GBM Team:
"At 00:08:39.16 UT on 14 May 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090514 (trigger 263952521 / 090514006).
The on-ground calculated location, using the GBM trigger
data, is RA = 12.3, DEC = -10.9 (J2000 degrees,
equivalent to 0 h 49 m, -10 d 54'), 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 is 19 degrees.
The GBM light curve consists of multiple peaks
with a duration (T90) of about 49 s (8-1000 keV).
The time-averaged spectrum from T0-1.5 s to T0+56.8 s is
adequately fit by a simple power law function with index -1.92 +/- 0.04.
The event fluence (8-1000 keV) in this time interval is
(8.1 +/- 0.2)E-06 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+0.256 s in the 8-1000 keV band
is 7.6 +/- 0.2 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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