{
  "submittedHow": "email-legacy",
  "eventId": "GRB 241026A",
  "circularId": 38028,
  "bibcode": "2024GCN.38028....1M",
  "subject": "GRB 241026A: SAO RAS optical observations",
  "submitter": "Moskvitin Alexander at SAO RAS <mosk@sao.ru>",
  "body": "A. S. Moskvitin, A. S. Vinokurov (SAO RAS), A. S. Pozanenko (IKI),\nN. Pankov (IKI, HSE) report on behalf of the GRB follow-up team.\n\nWe observed the field of GRB 241026A (The Fermi GBM team, GCN 37894;\nMelandri et al., GCN 37896, Li et al., GCN 37909; Zhang et al.,\nGCN 37921; Zhang, Xiong and Wang GCN 37924; Pal et al., GCN 37929;\nBarthelmy et al., GCN 37971) with the 6-m telescope of SAO RAS\nequipped with the focal reducer Scorpio-I on October 30,\n17:38:47--18:14:14 UT (t_mid-T0 = 3.8014 d).\n\nThe OT (Moskvitin et al., GCNs 37899, 37916, 37953; Watson et al.,\nGCN 37900; Zheng & Filippenko GCN 37903; Shrestha et al., GCN 37913;\nMo et al., GCN 37915; Mohan et al., GCN 37918; Izzo et al., GCN 37925;\nWang et al., GCN 37928, Rossi et al., GCN 37969) is detected\nin a stack image of  42 x 30 sec. The brightness of the OT is\nR = 23.9 +/- 0.2, calibrated against nearby USNO-B1.0 stars\n(R2 magnitudes) and not corrected for Galaxy extinction.\n\n",
  "createdOn": 1730455487044
}