TITLE: GCN CIRCULAR NUMBER: 38409 SUBJECT: EP241126a: SOAR observations of the optical counterpart DATE: 24/12/01 21:45:36 GMT FROM: James Freeburn at Swinburne University of Technology <jamesfreeburn54@gmail.com> J. Freeburn (Swinburne/OzGrav), I. Andreoni (UNC), J. Carney (UNC) We observed the optical counterpart to the X-ray transient, EP241126a (Hu et al., GCN 38335; Zheng et al., GCN 38339), with the Goodman High Throughput Spectrograph mounted on the SOAR telescope in imaging mode. We took three 300s exposures in r-band between 2024-11-28T03:48:34 and 2024-11-28T04:07:23 UTC corresponding to ~32 hours after the initial trigger. We detect the optical counterpart associated with EP241126a (Fu et al., GCN 38337; Li et al., GCN 38338; Geng et al., GCN 38357; Qiu et al., GCN 38378; Malesani et al., GCN 38385; Zou, GCN 38404). With photometric calibration using the Pan-STARRS1 catalogue, we measure r= 23.325 +/- 0.090 AB magnitude. View this GCN Circular online at https://gcn.nasa.gov/circulars/38409. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...