Physics & Spacearticle2026-09-26

The Gravitational-wave Optical Transient Observer (GOTO) Fast Analysis and Spectroscopy of Transients (FAST) Surveys

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Abstract

Abstract The study of young and fast astronomical transients is often limited by the difficulty of acquiring data, particularly spectra, within hours to days of explosion. Historically, follow-up programmes have rarely obtained spectra until many days after discovery; coupled with lower-cadence discovery observations, this has meant that the early evolution of transients has not been systematically probed. The Fast Analysis and Spectroscopy of Transients (FAST) programme aims to build a rich data set on the early evolution of a range of transients by linking a high-cadence discovery survey on the Gravitational-wave Optical Transient Observer (GOTO) with immediate visitor-mode spectroscopic follow-up. We report results from two prototype runs, FAST 23 and 24, carried out in August 2023 and February 2024 using the 2.54 m Isaac Newton Telescope. Between these, 51 transient classifications were reported, 19 of which were discovered by GOTO with a median time between discovery and first spectrum of < 2 days. We highlight the discovery and characterisation of SN 2024cld, enabled by spectroscopic observations beginning within 30 minutes of discovery, which reveals the complex mass-loss history of an evolved supergiant star in its final years prior to supernova. Further GOTO-FAST runs are ongoing at the Nordic Optical Telescope, and we hope this paper will be informative for those considering the creation of similar programmes.

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View paper (DOI)Open access versionOpenAlexMonthly Notices of the Royal Astronomical SocietyPublished 2026-09-26

Authors: B. Godson, J. D. Lyman, M. Pursiainen, Danny T. H. Steeghs, Benjamin D. R. Davies, Martin J. Dyer, N Koivisto, Michael K. Mitchell, D O’Neill, Bob Warwick, S Belkin, Paul Robin Brian Chote, D L Coppejans, Rob A. J. Eyles-Ferris, D Jarvis, Y Julakanti, L Kelsey, Mark R Kennedy, Thomas L. Killestein, A Kumar, A Levan, S Littlefair, M Magee, S Mandhai, D Mata Sánchez, S Mattila, J McCormac, J Mills, S Moran, J Mullaney, C Phillips, D Pollacco, K Pu, A Sahu, U Sawangwit, M Shrestha, E Stanway, R Starling, Yu-Zhu Sun, K Ulaczyk, L Vincetti, E Wickens, K Wiersema, D K Galloway, V. S. Dhillon, P O’Brien, Gavin Ramsay, K Noysena, R Kotak, R. P. Breton, L K Nuttall, Benjamin P. Gompertz, Jorge Casares

Institutions: University of Sheffield, University of Manchester, Monash University, University College Cork, Radboud University Nijmegen, University of Cambridge, University of Turku, University of Birmingham, European University Cyprus, University of Hertfordshire, University of Portsmouth, Universidad de La Laguna, University of Warwick, University of Leicester, The Open University, Armagh Observatory & Planetarium, Instituto de Astrofísica de Canarias, Institute of Astronomy, National Astronomical Research Institute of Thailand, Physical Sciences (United States), Institute for Globally Distributed Open Research and Education