TITLE: GCN CIRCULAR NUMBER: 41672 SUBJECT: EP/WXT01709201159: GOTO optical follow-up DATE: 25/09/03 15:13:59 GMT FROM: Ben Gompertz at U of Birmingham D. O'Neill, M. E. Wortley, B. P. Gompertz, A. Kumar, R. Starling, K. Ackley, M. J. Dyer, J. Lyman, K. Ulaczyk, B. Godson, D. Steeghs, D. K. Galloway, V. Dhillon, P. O'Brien, G. Ramsay, K. Noysena, R. Kotak, R. P. Breton, L. K. Nuttall, and J. Casares report on behalf of the GOTO collaboration: We report on optical observations with the Gravitational-wave Optical Transient Observer (GOTO; Steeghs et al. 2022, Dyer et al. 2024) in response to the EP/WXT trigger number 01709201159. A targeted observation was performed at Sept. 3 2025 14:10:33 UT, (+0.13h post trigger). The images were taken in the GOTO L-band (400-700 nm) and consisted of 4x90s exposures. Images were processed immediately after acquisition using the GOTO pipeline. Difference imaging was performed using deeper template observations. Source candidates were initially filtered using a classifier (Killestein et al. 2021) and cross-matched against a variety of contextual and minor planet catalogs. Human vetting was carried out in real time on any candidates that passed the above checks. We do not identify any candidate optical counterparts within the EP/WXT localisation uncertainty region after the trigger time, down to a 3-sigma limiting magnitude of L > 20.0 AB mag. Additionally, we do not see any evidence for stellar variability consistent with the WXT uncertainty region. Magnitudes were calibrated using ATLAS-REFCAT2 (Tonry et al. 2018) and were not corrected for Galactic extinction. GOTO (https://goto-observatory.org) is a network of telescopes that is principally funded by the STFC and operated at the Roque de los Muchachos Observatory on La Palma, Spain, and Siding Spring Observatory in NSW, Australia, on behalf of a consortium including the University of Warwick, Monash University, Armagh Observatory & Planetarium, the University of Leicester, the University of Sheffield, the National Astronomical Research Institute of Thailand (NARIT), the University of Turku, the University of Portsmouth, the University of Manchester and the Instituto de Astrofisica de Canarias (IAC).