{
  "submittedHow": "email",
  "createdOn": 1794351613543,
  "submitter": "Alexander Moskvitin at SAO RAS <mosk@sao.ru>",
  "body": "A. Moskvitin (SAO), O. Spiridonova (SAO), V. Rumyantsev (CrAO),\nA. Pozanenko (IKI), A. Volnova (IKI), N. Pankov (IKI) report\non behalf of SAO GRB follow-up team and IKI GRB-FuN.\n\nWe observed the field of the SVOM GRB 261110A (Wang et al., GCN 46215)\nwith the Zeiss-1000, 1-m telescope of SAO RAS on November 10,\n19:54:00--21:00:26 UT (t_mid - T0 = 8.62 hours after the trigger).\n\nThe OT (Wu et al., GCN 46218; Li et al., GCN 46219) is detected\nin our stacked frame with the following brightness.\n\nDate       UT start  t-T0     Exp,    Filter Obj      Err   UL\n                     (mid, d) (n*s)                         (3sigma)\n2026-11-10 19:54:00  0.35918  12*300  Rc     23.0 +/- 0.2   23.6\n\nThis preliminary photometry (Vega) is based on nearby SDSS stars\n(Lupton 2005 transformation) and not corrected for Galactic\nextinction.\n\n\n_____________________________________________\nAlexander Sergeevich Moskvitin, Ph. D., researcher,\nOptical Transient Physics Laboratory (#523), SAO RAS,\n369167, Nizhnij Arkhyz, Karachai-Cherkessia, Russia,\n+7(928)3946958, mosk@sao.ru\n",
  "subject": "GRB 261110A: SAO RAS optical observations",
  "circularId": 46220,
  "eventId": "GRB 261110A"
}