{
  "body": "N. Pankov (HSE, IKI), A. M. Abdelaziz (NRIAG), M. Abdelkareem (NRIAG), E. Amin (NRIAG), A. Pozanenko (IKI) report on behalf of IKI GRB-FuN:\n\nWe performed optical observations of the field of GRB 250226A (The Fermi GBM team, GCN 39479; V.Lipunov et. al, GCN 39481; Jiang et. al, GCN 39482; An et. al, GCN 39486; Zhu et. al, GCN 39487; Magnani et. al, GCN 39488; Li et. al, GCN 39489; Li et. al, GCN 39492; Aryan et. al, GCN 39509; Zou et. al, GCN 39511; Jiang et. al, GCN 39513; Li et. al, GCN 39514; Junjie-Jin et. al, GCN 39515; Thakur et. al, GCN 39518; Poidevin et. al, GCN 39524; Pathak et. al, GCN 39530; Pankov et. al, GCN 39539) in the R filter with the 1.88-meter telescope of the Kottamia Astronomical Observatory (KAO). The observations started on (UT) 2025-02-28 00:30:36, i.e. ~1.78 days since trigger and consists of 39x150 sec exposures. We do not detect the optical counterpart in the stacked image. The preliminary upper limit is as follows:\n\nDate       UT start  t-T0         Exp.    Filter  UL(3sigma)\n                     (mid, days)  (s)\n2025-02-28 00:30:36  1.78084      39*150  R        22.3\n\nThe photometry is based on nearby stars from the USNO-B1.0 catalog and has not been corrected for the Galactic extinction.",
  "eventId": "GRB 250226A",
  "format": "text/plain",
  "circularId": 39540,
  "createdOn": 1740775687053,
  "submittedHow": "web",
  "bibcode": "2025GCN.39540....1P",
  "submitter": "Nicolai Pankov at HSE, IKI RAS <colinsergesen@gmail.com>",
  "subject": "GRB 250226A: KAO Optical Upper Limit"
}