TITLE: GCN CIRCULAR NUMBER: 43816 SUBJECT: GRB 260223A: SVOM/VT optical observation DATE: 26/02/24 03:00:50 GMT FROM: Huali Li at at NAOC, SVOM <lhl@nao.cas.cn> H. L. Li, Y. N. Ma, L. P. Xin, Y. L. Qiu, C. Wu, Z. H. Yao, X. H. Han, Y. Xu, J. Wang, P. P. Zhang, W. J. Xie, Y. J. Xiao, H. B. Cai, L. Lan, J. R. Xu, J. S. Deng, J. Y. Wei (NAOC), J. Palmerio (CEA) report on behalf of the SVOM/VT team. SVOM/VT performed a Target of Opportunity observation of GRB 260223A detected by Fermi (Fermi GBM team et al., GCN 43808; Preis et al., GCN 43810) and SVOM/GRM (sb26022301, Wang et al., GCN 43815). The observation started on 2026-02-23T15:26:24 UTC, i.e. about 11.26 hours after the trigger time of GBM, in the VT_B (400nm-650nm) and VT_R (650nm-1000nm) channels simultaneously. The optical counterpart (Becerra et al., GCN 43811; Postigo et al., GCN 43812; Postigo et al., GCN 43814) were detected in both channels. The measurements in AB magnitude are derived as follows: Mid time | Band | Exposure Time | Magnitude (AB) 14.893 hours VT_R 27*70 sec 19.66 +/- 0.06 mag 14.864 hours VT_B 28*70 sec 20.50 +/- 0.08 mag The counterpart showed a power-law decay with the index of -1.1 during our observation from 11.40 hours to 15.14 hours. 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/43816. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...