TITLE: GCN CIRCULAR NUMBER: 17224 SUBJECT: GRB 141222A: First MASTER-SAAO optical observation DATE: 14/12/23 16:08:15 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs D.Buckley, S. Potter, A. Kniazev South African Astronomical Observatory E. Gorbovskoy,V. Lipunov, P.Balanutsa, D.Denisenko, M.Pruzhinskaya,A.Kuznetsov, V.Kornilov, D.Kuvshinov, N.Tyurina Lomonosov Moscow State University, Sternberg Astronomical Institute O.Gres, K.Ivanov, S.Yazev, N.M.Budnev, V.A.Poleshchuk Irkutsk State University V.Yurkov, Yu.Sergienko, D.Varda, E.Sinyakov Blagoveschensk Educational State University A. Tlatov, A.V. Parhomenko, D. Dormidontov, V.Sennik Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinsky, I.Zalozhnih, A. Popov Ural Federal University, Kourovka H. Levato and C. Saffe Instituto de Ciencias Astronomicas de la Tierra y del Espacio (ICATE), San Juan, Argentina C. Mallamacci, C. Lopez and F. Podest Observatorio Astronomico Felix Aguilar (OAFA), San Juan National University, Argentina MASTER II robotic telescope (MASTER-Net: http://observ.pereplet.ru) instaleted several days ago in South African Astronomical Observatory (Sutherland) automaticaly was pointed to the Fermi_LAT GRB141222A (McEnery et al., GCN 17218) after error box rised at 2014-12-22 22:34:35 UT (15.5 hours after trigger time) in unfiltered regime. Because we have no reference images we can only use DSS stars. There is no any optical transients brighter 20.8 unfiltered magnitude inside error box (between 2014-12-22 22:34:35 and 2014-12-23 00:26:09). We note that error box has small Galactic Latitude b = 4.3 but no very big absorption in R and I, they are 0.9 and 0.7 correspondently (Schlafly & Finkbeiner 2011, ApJ 737, 103). This message may be cited.