TITLE: GCN CIRCULAR NUMBER: 46122 SUBJECT: EP261030a: Global MASTER-Net observations report DATE: 26/10/31 22:09:49 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs D.Buckley (SAAO), V.Lipunov, E.Gorbovskoy, A.Kuznetsov, K.Zhirkov, I.Panchenko, N.Tiurina, P.Balanutsa, V.Topolev, D.Vlasenko, G.Antipov, A.Sankovich, Yu.Tselik, Ya..Kechin, V.Senik, A.Chasovnikov, K.Labsina (Lomonosov MSU) A. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity) A.Sosnovskij (Lomonosov MSU) A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory) L.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez, A.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory) R.Rebolo (The Instituto de Astrofisica de Canarias) O.Gress, N.Budnev(ISU) M. Segura, F. Podesta, R.Podesta, E. Gonzalez (Observatorio Astronomico Felix Aguilar (OAFA) MASTER-SAAO robotic telescope [1] located in South Africa (South African Astronomical Observatory) was pointed to the EP261030a ( EP Team at NAOC/CAS et al., GCN 46121) errorbox 37209 sec after notice time and 1 days 16553 sec after trigger time at 2026-10-31 21:51:12 UT, with upper limit up to 19.7 mag. The observations began at zenith distance = 21 deg. The sun altitude is -42.9 deg. The galactic latitude b = -71 deg., longitude l = 160 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=3532176 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 103013 | 2026-10-31 21:51:12 | MASTER-SAAO | (01h 32m 47.13s , -12d 01m 38.8s) | C | 120 | 19.2 | 103133 | 2026-10-31 21:51:12 | MASTER-SAAO | (01h 32m 47.13s , -12d 01m 38.8s) | C | 360 | 19.7 | Coadd 103013 | 2026-10-31 21:51:12 | MASTER-SAAO | (01h 30m 53.63s , -11d 45m 59.2s) | C | 120 | 19.1 | 103133 | 2026-10-31 21:51:12 | MASTER-SAAO | (01h 30m 53.63s , -11d 45m 59.2s) | C | 360 | 19.6 | Coadd 103166 | 2026-10-31 21:53:45 | MASTER-SAAO | (01h 32m 41.39s , -12d 02m 16.3s) | C | 120 | 19.0 | 103166 | 2026-10-31 21:53:45 | MASTER-SAAO | (01h 30m 47.87s , -11d 46m 35.7s) | C | 120 | 18.9 | 103319 | 2026-10-31 21:56:17 | MASTER-SAAO | (01h 30m 49.67s , -11d 45m 28.6s) | C | 120 | 19.0 | 103319 | 2026-10-31 21:56:17 | MASTER-SAAO | (01h 32m 43.18s , -12d 01m 09.7s) | C | 120 | 19.0 | 103471 | 2026-10-31 21:58:50 | MASTER-SAAO | (01h 32m 47.69s , -12d 02m 03.8s) | C | 120 | 19.0 | 103471 | 2026-10-31 21:58:50 | MASTER-SAAO | (01h 30m 54.16s , -11d 46m 22.4s) | C | 120 | 19.2 | 103623 | 2026-10-31 22:01:22 | MASTER-SAAO | (01h 32m 41.94s , -12d 02m 58.8s) | C | 120 | 19.7 | 103623 | 2026-10-31 22:01:22 | MASTER-SAAO | (01h 30m 48.39s , -11d 47m 17.2s) | C | 120 | 19.7 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. [1] - V.M. Lipunov, V.G. Kornilov, E.S. Gorbovskoy, N.A. Tiurina & A.S.Kuznetsov, 2023, Astronomical Robotic Networks and Operative Multichanel Astrophysics, Lomonosov MSU PRESS, 591pp. http : // www.pereplet.ru/lipunov/625.html