GCN Circular 33441
Subject
GRB 230204B: MASTER detection of an object near NTT Optical Afterglow Candidate
Date
2023-03-09T17:24:15Z (2 years ago)
From
Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov@xray.sai.msu.ru>
V.Lipunov (Lomonosov MSU), D.A.H.Buckley (SAAO), A.Chasovnikov, Ya.Kechin,
A.Kuznetsov, N.Tiurina, O.Gress, E.Gorbovskoy, G.Antipov, P.Balanutsa,
K.Zhirkov, D.Vlasenko, V.Senik, D.Kuvshinov,
V.Topolev, Yu.Tselik, D.Cheryasov, I.Gorbunov, Ya.Kechin (Lomonosov Moscow
State University, SAI, Physics Department);
C.Francile, R. Podesta, F. Podesta (Observatorio Astronomico Felix Aguilar of
San Juan National University of Argentina),
R. Rebolo, M. Serra (The Instituto de Astrofisica de Canarias),
L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez,
A.Corella,L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory),
N.M.Budnev (ISU,API),
A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo
Observatory),
A. Gabovich, V.Yurkov (Blagoveschensk Educational State University)
MASTER-SAAO robotic telescope (Global MASTER-Net http://observ.pereplet.ru,
Lipunov et al., 2010, Advances in Astronomy, v.2010, 30L)
center (Kozyrev et al. GCN 33425) at position Levan et al., GCN 33439
31 hours after trigger (22 30 43UT 1800 sec) ~20.2 (Unfiltered). The
position accuracity
is about ~ 1 pix =2".
But there is the Gaia star 3".3 offset with same magnitude.
No object in MPC.
The reduction will be continued.