TITLE: GCN CIRCULAR NUMBER: 42887 SUBJECT: GRB 251129A: SVOM/VT optical fading DATE: 25/11/29 05:41:54 GMT FROM: Huali Li at at NAOC, SVOM <lhl@nao.cas.cn> H. L. Li , L. P. Xin, Y. L. Qiu, C. Wu, Z. H. Yao, Y. N. Ma, X. H. Han, J. Wang, Y. Xu, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. Palmerio (CEA), W. J. Tan (IHEP), D. F. Kong (GXU) report on behalf of the SVOM/VT team. SVOM/VT performed an automatic slew to the field of GRB 251129A (sb25112901, Tan et al., GCN 42879). The observation stared at 2025-11-29T02:43:03 UTC, I.e., 658 seconds post trigger in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously. With the downloaded early X band data, the optical counterpart (Angulo et al. GCN 42880; Watson, GCN 42883; Wu et al., GCN 42882; Masi et al. GCN 42885) was clearly detected in both channels. The measurements are given below: Mid_time Band Exposure Time Magnitude (AB) 12.43 min VT_B 50 sec 18.16+/-0.03 mag 12.43 min VT_R 50 sec 17.89+/-0.03 mag 44.96 min VT_B 50 sec 19.11+/-0.04 mag 44.96 min VT_R 50 sec 18.80+/-0.03 mag It was fading with a slope of about 0.7 with a single power law. Our photometry was not corrected for Galactic extinction. The Space Variable Objects Monitor (SVOM) is a China-France joint mission led by the Chinese National Space Administration (CNSA, China), National Center for Space Studies (CNES, France) and the Chinese Academy of Sciences (CAS, China), which is dedicated to observing gamma-ray bursts and other transient phenomena in the energetic universe. VT was jointly developed by Xi'an Institute of Optics and Precision Mechanics (XIOPM), CAS and National astronomical observatories (NAOC), CAS. View this GCN Circular online at https://gcn.nasa.gov/circulars/42887. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...