TITLE: GCN CIRCULAR NUMBER: 36597 SUBJECT: GRB 240529A: further SAO RAS optical observations DATE: 24/06/02 13:30:58 GMT FROM: Moskvitin Alexander at SAO RAS <mosk@sao.ru> A. S. Moskvitin, O. I. Spiridonova, O. A. Maslennikova (SAO RAS), report on behalf of the GRB follow-up team. We observed the field of the GRB 240529A (Eyles-Ferris et al. GCN 36556; Osborne et al. GCN 36557; Joshi et al. GCN 36560; Dichiara et al. GCN 36564; Markwardt et al. GCN 36566; Tan et al. GCN 36578) with the SAO RAS 1m telescope Zeiss-1000 equipped with CCD-photometer. We obtained 8 x 300 sec frames in the Rc band on June 1, 23:30:20 -- June 2, 00:16:50 UT (t_mid - T0 = 3.8716 days). The OT (Kumar et al. GCN 36559; Fu et al. GCN 36561; Shilling et al. GCN 36562; Perez-Garcia et al. GCN 36563; Dutton et al. GCN 36568; Mo et al. GCN 36569; Odeh et al. GCNs 36573, 36592; de Ugarte Postigo et al. GCN 36574; Adami et al. GCN 36575; Mohan et al. GCN 36576; Vinko et al. GCN 36577; Lim et al. GCN 36579; Pankov et al. GCN 36585; Ror et al., 36589) is clearly detected in the stacked frame with the brightness of R = 20.7 +/- 0.1. The magnitudes were calibrated using R2 magnitudes of nearby USNO-B1.0 stars. View this GCN Circular online at https://gcn.nasa.gov/circulars/36597. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...