GRB 090815
GCN Circular 9812
Subject
GRB 090815: Fermi GBM detection
Date
2009-08-15T13:11:29Z (16 years ago)
From
Andreas von Kienlin at MPE <azk@mpe.mpg.de>
A. von Kienlin (MPE) reports on behalf of the Fermi GBM Team:
"At 07:12:12.45 UT on 15 August 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090815 (trigger 272013134 / 090815300).
The on-ground calculated location, using the GBM trigger
data, is RA = 41.7, DEC = -2.0 (J2000 degrees, equivalent
to 02h 47m, -02d 00'), with an uncertainty of 7.6 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 87 degrees.
The GBM light curve shows two broad pulses with a duration
(T90) of about 200 s (8-1000 keV). The time-averaged spectrum
from T0-5.120 s to T0+24.576 s is well fit by a simple power
law function with index -1.5 +/- 0.1 (chi squared 261 for 241 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(3.4 +/- 0.3)E-06 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0+ 3.072 s in the 8-1000 keV band
is 1.9 +/- 0.3 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
GCN Circular 10025
Subject
GRB 090815: a faint long GRB localized by INTEGRAL
Date
2009-10-16T13:22:55Z (16 years ago)
From
Carlo Ferrigno at IAAT/ISDC <carlo.Ferrigno@unige.ch>
C. Ferrigno (ISDC, Versoix/IAAT, Tuebingen), D.Gotz (CEA-Saclay),
S.Mereghetti, A.Paizis (IASF-Milano), E. Bozzo, M. Beck (ISDC,
Versoix), and J.Borkowski (CAMK, Torun) on behalf of the IBAS
Localization Team report:
A faint long GRB with duration of about 100 s has been detected by
IBAS in IBIS/ISGRI data at 23:00:17 UTC on August 15th. No automatic
alert has been issued because the trigger was at low significance.
Interactive off-line analysis has allowed to confirm the GRB nature of
the trigger.
The refined coordinates (J2000) are:
RA: 306.13 [degrees] DEC: -6.17 [degrees]
with an uncertainty of 3 arcmin (90% c.l.).
The soft spectrum of the GRB (only detected in the 20-40 keV energy
range) and the long, slowly rising light curve may indicate a highly
redshifted burst. Follow-up observations at other wavelengths are
encouraged.
The light curve of the GRB will be posted at http://ibas.iasf-milano.inaf.it/IBAS_Results.html
This message can be cited.
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Carlo Ferrigno Institut f�r Astronomie
und Astrophysik T�bingen (IAAT)
and
ISDC Data Centre for Astrophysics
Chemin d'�cogia 16
CH-1290 Versoix Switzerland
Office +41.22.3792178
mobile (IT) +39.333.3599421
mobile (CH) +41.78.9210855
E-mail: Carlo.Ferrigno@unige.ch
Home Page: http://www.ifc.inaf.it/~ferrigno/
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