{
  "submittedHow": "email-legacy",
  "circularId": 38032,
  "eventId": "GRB 241030A",
  "body": "A. S. Moskvitin (SAO RAS) and V. P. Goranskij (SAI MSU)\nreport on behalf of the GRB follow-up team.\n\nWe observed the field of GRB 241030A / EP241030a (Klingler et al.,\nGCN 37956; Beardmore et al., GCN 37962; Wang et al., GCN 37972;\nPillera et al., GCN 37979; Ridnaia et al., GCN 37982; Ambrosi et al.,\nGCN 37988; Wu et al., GCN 37997; Liang et al., GCN 38026)\nwith the 1-m telescope of SAO RAS, Zeiss-1000 equipped\nwith the CCD-photometer on October 31, 17:49:28--18:22:41 UT\n(t_mid - T0 = 1.5125 days = 36.3 hours).\n\nThe OT (Klingler et al., GCN 37956; Watson et al., GCN 37957;\nFernández-Rodríguez et al., GCN 37958; Zheng et al., GCN 37959;\nAn et al., GCN 37960; Higuchi et al., GCN 37963; Qiu et al.,\nGCN 37965; Lin et al., GCN 37966; Wu et al., GCN 37970;\nBreeveld & Klingler, GCN 37974; Méndez-Lapido et al., GCN 37993;\nMoskvitin & Goranskij, GCN 38016; Busmann et al., GCN 38019;\nSchneider et al., GCN 38021; Li et al., GCN 38027; Masi, GCN 38031)\nis clearly detected in our 3 x 600 sec stacked frame in Rc band\nwith the brightness of R = 20.31 +/- 0.06 (R_lim = 22.6),\ncalibrated against nearby Pan-STARRS stars (magnitudes converted\nwith Lupton 2005 equations) and not corrected by MW extinction.\n\n",
  "submitter": "Moskvitin Alexander at SAO RAS <mosk@sao.ru>",
  "subject": "GRB 241030A: further SAO RAS optical observations",
  "bibcode": "2024GCN.38032....1M",
  "createdOn": 1730461727029
}