GCN Circular 21091
Subject
GRB 170510A: Global MASTER Net possible OT observations
Event
Date
2017-05-12T14:36:50Z (8 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov@xray.sai.msu.ru>
V. Lipunov, E. Gorbovskoy, V.Kornilov, N.Tyurina, D.Kuvshinov, A.V.Krylov,
I.Gorbunov, P.Balanutsa, A.Kuznetsov, V.V.Chazov, D. Vlasenko
Lomonosov Moscow State University, Sternberg Astronomical Institut
D.Buckley, S. Potter, A.Kniazev, M.Kotze
South African Astronomical Observatory
R.Podesta, C.Lopez, F. Podesta Observatorio Astronomico Felix Aguilar (OAFA) ,
National University of San Juan, Argentina
H. Levato, C. Saffe
Instituto de Ciencias Astronomicas,de la Tierra y del Espacio (ICATE),
San Juan, Argentina
K.Ivanov, S.Yazev, N.M.Budnev, O.Gres, O.Chuvalaev, V.A.Poleshchuk, O. Ershova
Irkutsk State University
V.Yurkov, Yu.Sergienko
Blagoveschensk Educational State University, Blagoveschensk
A. Tlatov, V.Senik, A.V. Parhomenko, D. Dormidontov
Kislovodsk Solar Station of the Pulkovo Observatory
R. Rebolo, M. Serra, N. Lodieu, G. Israelian, L. Suarez-Andres
The Instituto de Astrofisica de Canarias
MASTER-SAAO robotic telescope (MASTER-Net: http://observ.pereplet.ru) located
in SAAO was starting survey on the LAT GRB170510.22 error-box (Bissaldi et
al., GCN #21080) 22480 sec after notice time and 41530 sec after trigger time
at 2017-05-10 16:44:36 UT. The 5-sigma upper limit on our first (180s exposure)
set is about 18.9 mag
We marginaly see optical candidate (Cucchiara et al. GCN 21087) at XRT
(Evans et al. GCN #21082, Melandri et al. GCN #21086) position with
unfiltered mag ~ 19 m .
Ra, Dec = 10 40 36.76 -39 12 43.8 (+/-1 arcsec)
We did not see object 2.5 hours late with limit 19.5 .
So X-ray Source 1 (Melandri et al. GCN #21086) is possible OT.
The message may be cited.