[vsnet-grb-info 17652] GRB 160225A: MASTER-Amur observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Feb 26 18:28:46 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19089
SUBJECT: GRB 160225A: MASTER-Amur observations
DATE: 16/02/26 09:27:38 GMT
FROM: Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov at xray.sai.msu.ru>
N.Tyurina, E. Gorbovskoy, V. Lipunov, V.Kornilov, P.Balanutsa,
A.Kuznetsov, D.Kuvshinov
Lomonosov Moscow State University,
Sternberg Astronomical Institute, Moscow State University
A.Gabovich, V.Yurkov, Yu.Sergienko, D.Varda
Blagoveschensk Educational State University, Blagoveschensk
D.Buckley, S. Potter, M.Kotze
South African Astronomical Observatory
K.Ivanov, N.M.Budnev, O.Gres, V.A.Poleshchuk
Irkutsk State University
A. Tlatov, V.Senik, A.V. Parhomenko, D. Dormidontov
Kislovodsk Solar Station of the Pulkovo Observatory
R. Rebolo, M. Serra-Ricart, N. Lodieu, G. Israelian
The Instituto de Astrofisica de Canarias
MASTER II robotic telescope (MASTER-Net: http://observ.pereplet.ru)
located in Blagoveschensk was pointed to the GRB160225A 20 sec after
notice time and 204 sec after Swift BAT trigger (Siegel et al, 19075)
time at 2016-02-25 14:24:20 UT (Gabovich et al, 19076).
We did not see any OT brighter 2-sigma. Our unfiltered camera sensitive up
to 10 mk.
Id t_start-t_trigger t_mean-t_trig Exp.time Limit
s s s unfiltered
767291 204 224 40 17.4
767293 256 281 50 17.6
767295 318 348 60 17.0
769139 318 768 600 18.7
769244 318 1187 1200 19.0
Our unfiltered magnitude calibrated to USNOB1 stars as m =0.2B + 0.8R .
The message may be cited.
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