GCN Circular 16043
Subject
GRB 140320D: MASTER optical observations
Date
2014-03-30T08:42:43Z (11 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <gcncirc@observ.inetcomm.ru>
K.Ivanov, S.Yazev, N.M.Budnev, O.Gres, O.Chuvalaev, V.A.Poleshchuk
Irkutsk State University
E. Gorbovskoy, V. Lipunov, M. Pruzhinskaya, D.Denisenko, V.Kornilov, N.Tyurina,
P.Balanutsa, A.Kuznetsov, V.V.Chazov, D.Kuvshinov
Lomonosov Moscow State University, Sternberg Astronomical Institute
V.Yurkov, Yu.Sergienko, D.Varda, E.Sinyakov
Blagoveschensk Educational State University, Blagoveschensk
A. Tlatov, A.V. Parhomenko, D. Dormidontov, V.Sennik
Kislovodsk Solar Station of the Pulkovo Observatory
V.Krushinski, I.Zalozhnih, A. Popov
Ural Federal University, Kourovka
Hugo Levato and Carlos Saffe
Instituto de Ciencias Astronomicas, de la Tierra y del Espacio (ICATE)
Claudio Mallamaci, Carlos Lopez and Federico Podest
Observatorio Astronomico Felix Aguilar (OAFA)
MASTER II robotic telescope located in Tunka (MASTER-Net:
http://observ.pereplet.ru) have done a survey of the large area
around IPN error box (Hurley et. al. GCN16023). The survey was started
2014-03-21 13:15:06 i.e. 16h 53m after the burst and proceeded during 5
hours. The 5 sigma unfiltered upper limit was ~17.5 m on single
180 image and ~18.8 m on coadd of 5 images with total exposure 900 s.
We haven`t found credible optical afterglow candidate within IPN error box.
The covarege map is available at
http://master.sai.msu.ru/static/GRB/GRB140320D_map.png
The message may be cited.