GRB 190704A
GCN Circular 25024
Subject
IPN triangulation of GRB 190704A (short)
Date
2019-07-07T20:59:48Z (6 years ago)
From
Dmitry Svinkin at Ioffe Institute <svinkin@mail.ioffe.ru>
D. Svinkin, S. Golenetskii, R. Aptekar, D. Frederiks, A. Kozlova,
and T. Cline on behalf of the Konus-Wind team,
K. Hurley, on behalf of the IPN,
A. von Kienlin, X. Zhang, A. Rau, V. Savchenko, E. Bozzo,
and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team,
S. Barthelmy, J. Cummings, H. Krimm, and D. Palmer,
on behalf of the Swift-BAT team,
The short-duration GRB 190704A has been detected by Konus-Wind,
INTEGRAL (SPI-ACS trigger 8323) and Swift (BAT), so far,
at about 22353 s UT (06:12:33).
The burst was outside the coded field of view of the BAT.
We have triangulated it to a preliminary, 3 sigma error box
whose coordinates are:
---------------------------------------------
RA(2000), deg Dec(2000), deg
---------------------------------------------
Corners:
329.352 (21h 57m 25s) +48.888 (+48d 53' 15")
328.224 (21h 52m 54s) +47.140 (+47d 08' 24")
240.886 (16h 03m 33s) -1.156 ( -1d 09' 23")
242.721 (16h 10m 53s) -1.662 ( -1d 39' 42")
---------------------------------------------
The error box area is 175 sq. deg, and its maximum
dimension is 88.2 deg (the minimum one is 57.1 arcmin).
The Sun distance was greater than ~100 deg.
This box may be improved.
Fermi-GBM was enabled at the time of the GRB according to
glg_poshist_all_190704_v00.fit, so the non-detection by GBM
implies that the burst was Earth-Occulted for Fermi.
This burst is spatially and temporally inconsistent with IceCube-190704A
(The IceCube Collaboration, GCN Circ. 24981) and Baksan Neutrino
Observatory Alerts on 2019-07-03 (Lipunov et al., GCN Circ. 24976
and 24980).
A triangulation map is posted at
http://www.ioffe.ru/LEA/GRBs/GRB190704_T22351/IPN
The time history and spectrum will be given in forthcoming
GCN Circulars.
GCN Circular 25032
Subject
Konus-Wind observation of GRB 190704A
Date
2019-07-08T13:14:30Z (6 years ago)
From
Anastasia Tsvetkova at Ioffe Institute <tsvetkova@mail.ioffe.ru>
A. Tsvetkova, S. Golenetskii, R.Aptekar, D. Frederiks,
M. Ulanov, D. Svinkin, A. Lysenko, A. Kozlova and T. Cline
on behalf of the Konus-Wind team, report:
The short-duration, hard-spectrum
(IPN triangulation: Svinkin et al., GCN 25024)
triggered Konus-Wind at T0=22355.497 s UT (06:12:35.497).
The burst light curve shows a pulse with a duration of ~1.5 s
followed by a weaker pulse at ~T0+3.0.
The emission is seen up to ~16 MeV.
As observed by Konus-Wind, the burst
had a fluence of 3.56(-1.26,+3.48)x10^-6 erg/cm2,
and a 64-ms peak energy flux, measured from T0-0.310 s,
of 5.03(-2.48,+6.16)x10^-6 erg/cm2/s
(both in the 20 keV - 10 MeV energy range).
The time-integrated spectrum of the burst
(measured from T0 to T0+0.256 s)
is best fit in the 20 keV - 16 MeV range
by a power law with exponential cutoff model:
dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)
with�� alpha = -0.72(-0.41,+0.63),
and Ep = 861(-420,+2298) keV (chi2 = 21/20 dof).
The Konus-Wind light curve of this GRB is available at
http://www.ioffe.ru/LEA/GRBs/GRB190704_T22355/
All the quoted errors are at the 90% confidence level.
All the quoted values are preliminary.