{
  "eventId": "GRB 250214A",
  "subject": "Fermi GRB 250214A: Global MASTER-Net observations report",
  "submittedHow": "email",
  "body": "V.Lipunov, E.Gorbovskoy, N.Tiurina,  P.Balanutsa, , D.Vlasenko, I.Panchenko,\nA.Kuznetsov,  G.Antipov,  A.Sankovich, A.Sosnovskij, Yu.Tselik, M.Gulyaev, Ya.Kechin,\nV.Senik, A.Chasovnikov, K.Labsina, I. Gorbunov (Lomonosov MSU),\nO.Gress, N.Budnev (ISU),\nC.Francile,  F. Podesta, R.Podesta, E. Gonzalez  (Observatorio Astronomico Felix Aguilar (OAFA),\nA. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory),\nA. Gabovich, V.Yurkov (Blagoveschensk Educational StateUniversity)\nD.Buckley (SAAO),\nR.Rebolo (The Instituto de Astrofisica de Canarias),\nL.Carrasco, J.R.Valdes, V.Chavushyan, V.M.Patino Alvarez, J.Martinez,\nA.R.Corella, L.H.Rodriguez (INAOE, Guillermo Haro Astrophysics Observatory) \n\nMASTER-OAFA robotic telescope  (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L)  located in Argentina (OAFA observatory of San Juan National University) started inspect of the Fermi GRB 250214A ( Fermi GBM team, GCN 39320) errorbox  560 sec after notice time and 594 sec after trigger time at 2025-02-14 05:42:01 UT, with upper limit up to  19.1 mag. The observations began at zenith distance = 30 deg. The sun  altitude  is -44.1 deg. \n\nThe galactic latitude b = -4 deg., longitude l = 259 deg.\n\n\nReal time updated cover map and OT discovered available here: \nhttps://master.sai.msu.ru/site/master2/observ.php?id=2777807\n\nWe obtain a following upper limits.  \n\nTmid-T0  |      Date Time      |          Site       |             Coord (J2000)          |Filt.| Expt. | Limit| Comment\n_________|_____________________|_____________________|____________________________________|_____|_______|_______|________\n\n     644 | 2025-02-14 05:42:01 |         MASTER-OAFA | (08h 23m 56.50s , -41d 11m 58.0s) |   C |   100 | 18.2 |        \n     655 | 2025-02-14 05:42:01 |         MASTER-OAFA | (08h 11m 47.16s , -41d 33m 12.7s) |   C |   120 | 19.1 |        \n     781 | 2025-02-14 05:44:07 |         MASTER-OAFA | (08h 23m 56.66s , -41d 11m 56.7s) |   C |   120 | 18.3 |        \n     791 | 2025-02-14 05:44:08 |         MASTER-OAFA | (08h 11m 47.35s , -41d 33m 11.9s) |   C |   140 | 19.1 |        \n     942 | 2025-02-14 05:46:34 |         MASTER-OAFA | (08h 23m 56.87s , -41d 11m 55.7s) |   C |   150 | 18.3 |        \n     952 | 2025-02-14 05:46:34 |         MASTER-OAFA | (08h 11m 47.60s , -41d 33m 11.2s) |   C |   170 | 19.0 |        \n    1123 | 2025-02-14 05:49:30 |         MASTER-OAFA | (08h 23m 57.07s , -41d 11m 55.2s) |   C |   160 | 18.4 |        \n    1133 | 2025-02-14 05:49:30 |         MASTER-OAFA | (08h 11m 47.85s , -41d 33m 10.2s) |   C |   180 | 18.8 |        \nFilter C is a clear (unfiltred) band. \n\n\nThe observation and reduction will continue. \nThe message may be cited.\n",
  "submitter": "Vladimir Lipunov at Moscow State U/Krylov Obs <lipunov@xray.sai.msu.ru>",
  "bibcode": "2025GCN.39322....1L",
  "circularId": 39322,
  "createdOn": 1739527396230
}