{
  "body": "J. Y. Wei, L. P. Xin, Y. Xu, J. R. Xu, X. H. Han, H. L. Li, J. Wang, L. Huang, Y. L. Qiu, L.J. Wang, H. B. Cai,  C. Wu, L. J. Chen, Y. T. Zheng, W. L. Dong, P. P. Zhang, Y. J. Xiao , Y. N. Ma , S., Jin, Z. R. Cui, W. J. Xie, J. S. Deng (NAOC), Z. G. Dai (USTC), X. Y. Wang (NJU), E. W. Liang (GXU), X. G. Wang (GXU) report on behalf of SVOM/GWAC team.\n\nThe field of GRB 261113A triggered by SVOM/Eclairs (sb26111302, Saccardi et al., GCN 46244, Dagoneau et al., GCN 46270) was monitored by GWAC system continuously during about 4 hrs before and 12 minutes post trigger. The exposure time for each frame is 3 sec.\n\nThe optical counterpart (Lin et al., GCN 46247; Lei et al., GCN 46248; Li et al., GCN 46249; Yin et al., GCN 46250; Chen et al., GCN 46251; Wu et al., GCN 46252; Zhao et al., GCN 46253; Li et al., GCN 46254; Saikia et al., GCN 46256; Adami et al., GCN 46257; Gress et al., GCN 46258; Izzo et al., GCN 46259; Brivio et al., GCN 46260; Maksut et al., GCN 46262; Moskvitin et al., GCN 46263; Perez-Garcia et al., 46264; Dimple et al., GCN 46266; Jelinek et al., GCN 46271) was clearly detected in single frames with a peak brightness of W~11 mag at around 10 seconds after the burst. The magnitude is calibrated to the GAIA G-band and not corrected for Galactic extinction.",
  "editedOn": 1794686892858,
  "submittedHow": "web",
  "subject": "GRB 261113A: SVOM/GWAC bright optical counterpart",
  "format": "text/plain",
  "editedBy": "K.L. Page at U Leicester <klp5@leicester.ac.uk> on behalf of Huali Li at at NAOC, SVOM <lhl@nao.cas.cn>",
  "eventId": "GRB 261113A",
  "circularId": 46274,
  "submitter": "Liping Xin at NAOC, SVOM <xlp@nao.cas.cn>",
  "createdOn": 1794668015058,
  "eventType": [
    "GRB",
    "X-ray Transient",
    "Optical Transient"
  ],
  "version": 2
}