TITLE: GCN CIRCULAR NUMBER: 24370 SUBJECT: GRB 190501A: GOTO optical counterpart search DATE: 19/05/02 16:52:17 GMT FROM: Danny Steeghs at U.of Warwick/GOTO J.Lyman(1), K.Ulaczyk(1), K.Wiersema(1), D.Steeghs(1), M.Dyer(3), D.Galloway(2), V.Dhillon(3), P.O'Brien(4), G.Ramsay(5), D.Pollacco(1), E.Thrane(2), S.Poshyachinda(6), E.Palle(7), R.Cutter(1), A.Levan(1), T. Marsh(1), R.West(1), B.Gompertz(1), E.Stanway(1), K.Ackley(2), A.Obradovic(2), Y-L.Mong(2), A.Casey(2), M.Brown(2), E.Rol(2), J.Mullaney(3), S.Littlefair(3), L.Makrygianni(3), E.Daw(3), J.Maund(3), R.Starling(4), R.Eyles(4), S.Tooke(4), U.Sawangwit(6), D.Mkrtichian(6), S.Awiphan(6), S.Aukkaravittayapun(6), P.Irawati(6), M.Kennedy(8), R.Breton(8), D.Mata-Sanchez(8), T.Heikkila(9), R.Kotak(9) (1) Warwick University; (2) Monash University; (3) Univ. of Sheffield; (4) University of Leicester; (5) Armagh Observatory & Planetarium; (6) National Astronomical Research Institute of Thailand; (7) Instituto de Astrofisica de Canarias; (8) Univ. of Manchester; (9) University of Turku report on behalf of the GOTO collaboration: We report on optical observations with the Gravitational-wave Optical Transient Observer in response to the AGILE detected GRB 190501A (Ursi et al. GCN #24360). The refined position reported in Verrecchia et al. (GCN #24363) was covered with a set of 5x90s exposures starting at 2019-05-01T20:49 (15.4 hours after the burst) using our wide L filter (400-700 nm). No viable counterpart is detected using a difference imaging analysis based on recent survey observations of the same pointing. We achieved a 5-sigma detection limit of g=20, based on a photometric calibration against PS1 stars. GOTO is operated at the La Palma observing facilities of the University of Warwick on behalf of a consortium including the University of Warwick, Monash University, Armagh Observatory, the University of Leicester, the University of Sheffield, the National Astronomical Research Institute of Thailand (NARIT) and the Instituto de Astrofisica de Canarias (IAC) (https://goto-observatory.org/)