WFST Discovered Two Optical Counterpart Candidates of GRB231110A

Following the detection of GRB 231110A by SWIFT (D’Elia et al., GCN 34977) and MASTER (Lipunov et al., GCN 34978), WFST observed the target position with 13x60s and 27x90s exposure in i-band starting from 10 Nov 2023, UTC 05:59:01, about 39.45 minutes after the burst. After stacking the individual exposures (5x90s) to enhance observation depth, WFST found two possible candidates.

Refer https://gcn.nasa.gov/circulars/34979 for more details.