GRB 241217A: GMG Optical Upper Limit

We observed the field of GRB 241217A (Marius et al., GCN 38594, T0 at 2024-12-17T16:57:13) using the GMG-2.4m telescope at the Lijiang Observatory. The observation began at 2024-12-17T17:30:55, about 0.56 hours after the trigger. No new uncataloged optical source was detected within the SVOM/VT error circle (GCN 38600). The preliminary analysis results are shown as follows: +----------------+------------+----------+----------------+ | Tmid-T0 [hr] | Exp. [s] | Filter | 5-sigma U.L. | +================+============+==========+================+ | 0.65 | 600 | r | 20.6 | +----------------+------------+----------+----------------+ The given magnitudes are derived based on calibrating against Pan-STARRS1 field stars.