TITLE: GCN CIRCULAR NUMBER: 21499 SUBJECT: LIGO/Virgo G297595: MASTER MASTER Bright PSN detection in error-box DATE: 17/08/16 18:33:47 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs V.M. Lipunov, E. Gorbovskoy, V.G.Kornilov, N.Tyurina, V.Shumkov, D.Kuvshinov, P.Balanutsa, O.Gress, A.Kuznetsov, M.I.Panchenko, A.V.Krylov, I.Gorbunov Lomonosov Moscow State University, Sternberg Astronomical Institute 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 N.M. Budnev, O. Gress, K. Ivanov, S.Yazev Irkutsk State University V.Yurkov, Yu.Sergienko, A.Gabovich Blagoveschensk Educational State University, Blagoveschensk D.Buckley, S. Potter, M. Kotze, South African Astronomical Observatory R. Rebolo, M. Serra-Ricart, G. Israelian, N.Lodiu The Instituto de Astrofisica de Canarias A. Tlatov, V.Sennik Kislovodsk Solar Station of the Pulkovo Observatory Following Katsavounidis et al. (GCN 21474), we report two optical transients detected. 1) MASTER OT J030141.96-230037.8 discovery During MASTER-OAFA inspection of LIGO GW G297595 MASTER-OAFA auto-detection system ( Lipunov et al., "MASTER Global Robotic Net", Advances in Astronomy, 2010, 30L ) discovered OT source at (RA, Dec) = 03h 01m 41.96s -23d 00m 37.8s on 2017-08-16.31422 UT. The OT unfiltered magnitude is 17.5m (mlim=19.7m). The OT is seen in 2 image (MASTER inspection mode) at 2017-08-16 07:32:29 and 2017-08-16 07:17:07UT There is no minor planet at this place. We have reference images without OT on 2017-03-10.01 UT with magnitude limit in unfiltered 18.6m. Spectral observations are required. The discovery and reference images are available at:http://master.sai.msu.ru/static/OT/030141.96-230037.8.png 2) MASTER OT J015849.50-230853.7 detection MASTER-OAFA auto-detection system discovered OT source at (RA, Dec) = 01h 58m 49.50s -23d 08m 53.7s on 2017-08-15.27118 UT. The OT unfiltered magnitude is 16.7m (mlim=19.3m). The OT is seen in 3 images. There is no minor planet at this place. We have reference image without OT on 2016-09-22.25362 UT with unfiltered magnitude limit is 18.4m. There is USNO-B1 star in 2" with known only B1=21.47,B2=20.96 Spectral observations are required. The discovery and reference images are available at: http://master.sai.msu.ru/static/OT/015849.50-230853.7.png This message can be citted.