[vsnet-grb-info 16760] GRB 150721A: Fermi GBM detection

[GCN Circulars]

TITLE:   GCN CIRCULAR
NUMBER:  18041
SUBJECT: GRB 150721A: Fermi GBM detection
DATE:    15/07/21 20:55:52 GMT
FROM:    Elisabetta Bissaldi at U.Innsbruk/IAPP  <Elisabetta.Bissaldi at uibk.ac.at>

E. Bissaldi (INFN Bari), V. Connaughton (USRA) and
A. von Kienlin (MPE) report on behalf of the Fermi GBM Team:


At 05:49:08.93 UT on 21 July 2015, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 150721A (trigger 459150552/150721242).

The on-ground calculated location, using the GBM trigger
data, is

RA= 334.1, DEC = +7.8
(J2000 degrees, equivalent to 22h 16m, 07d 48')

with an uncertainty of 1.5 degrees (radius, 1-sigma containment,
statistical only; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).

The trigger resulted in an Autonomous Repoint Request (ARR)
by the GBM Flight Software owing to the high peak flux of the GRB.
This was accepted and the spacecraft slewed to the GBM in-flight
location. The initial angle from the Fermi LAT boresight
is 63 degrees.

This burst was also independently detected by INTEGRAL SPI-ACS.

The GBM light curve consists of a first peak at trigger
time followed by a very soft peak around 100 s.
The duration (T90) is about 20 s (50-300 keV).
The time-averaged spectrum from T0 to T0+20.2 s
is best fit by a smoothly broken power law function.
The low-energy index is -0.58 +/- 0.06, the high-energy
index is -2.90 +/- 0.06 and the break energy
is 45.7 +/- 2.3 keV.

The event fluence (10-1000 keV) in this time interval is
(1.52 +/- 0.08)E-05 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+5.4 s in the 10-1000 keV band
is 16.7 +/- 0.3 ph/s/cm^2.

A Band function fits the spectrum equally well
with Epeak = 56.26 +/- 1.15 keV,
alpha = -0.16 +/- 0.07, and beta = -2.74 +/- 0.05.


The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog.