TITLE: GCN CIRCULAR NUMBER: 37271 SUBJECT: GRB 240824A: SVOM/C-GFT optical upper limit DATE: 24/08/25 14:38:45 GMT FROM: Chao Wu at NAOC SVOM/C-GFT team: Chao WU (NAOC), Zhe Kang (CHO),Liping Xin(NAOC),Xuhui Han(NAOC),Pinpin Zhang (NAOC),Xiaomeng Lu (NAOC), Zhenwei Li (CHO),You Lv (CHO),Ruosong Zhang (NAOC),Yujie Xiao(NAOC) SVOM JSWG: Jian-Yan Wei (NAOC, China), Bertrand Cordier (CEA, F), Shuang-Nan Zhang (IHEP, CN), Stephane Basa (LAM, F), Jean-Luc Attéia (IRAP, F), Arnaud Claret (CEA, F), Zi-Gao Dai (USTC, CN), Frederic Daigne (IAP, F), Jin-Song Deng (NAOC, CN), Andrea Goldwurm (APC, F), Diego Götz (CEA, F), Xu-Hui Han (NAOC, CN), Cyril Lachaud (APC, F), En-Wei Liang (GXU, CN), Yu-Lei Qiu (NAOC, CN), Susanna Vergani (Obs. Paris, F), Jing Wang (NAOC, CN), Chao Wu(NAOC, CN), Li-Ping Xin (NAOC, CN), Bing Zhang (UNLV, CN) We observed the field of the Swift GRB 240824A (Cenko et al., GCN 37254) starting at 11:02:55UT, August 24, 2024, ~10 hr after the burst with C-GFT (Chinese Ground Follow-up Telescope in SVOM mission) in System Test Mode (STM). C-GFT is located at Jilin (long.=126.33 deg, lat.= 43.8243778 deg), Changchun Observatory, National Astronomical Observatories, CAS. It has FOV of 1.28 deg X 1.28 deg with a 4k*4k CMOS detector mounted on the primary focus of 1.2-meter-aperure telescope. A series of g ,r,and i band images were obtained. We obtained stacked images of r: 245 x 10s,g: 255 x 10s and i:234 x 10s. No optical afterglow was detected for the candidate reported by Evans (GCN 37269) down to the limit magnitude of mag_g=20.6 , mag_r=20.5, and mag_i=20.0. The photometry was calibrated with UCAC4 catalogs. We thank the observation assistant Bowen Li at Jilin observatory for their excellent support.