TITLE: GCN CIRCULAR NUMBER: 32289 SUBJECT: GRB 220627A: MeerLICHT candidate optical afterglow DATE: 22/06/28 22:59:47 GMT FROM: Simon de Wet at UCT S. de Wet (UCT), P.J. Groot (Radboud/UCT/SAAO), D.B. Malesani (Radboud and DAWN/NBI), A.J. Levan (Radboud) and D. Pieterse (Radboud) report on behalf of the MeerLICHT consortium: Following the Fermi/LAT detection and localisation of GRB 220627A (Di Lalla et al., GCN 32283), also proposed to be a lensed or ultra-long GRB candidate by Fermi/GBM (Roberts et al., GCN 32288), the 0.6 m wide-field MeerLICHT optical telescope obtained 2x300s observations in the q-band of two fields encompassing the LAT error box starting at 17:12:15 UT on 2022 June 28, approximately 1.17 days after the GBM trigger. We note that these two fields were not observed during observations of the Fermi/GBM error box from the previous night (Groot et al., GCN 32281). We also note that the two transient candidates from those observations are not consistent with the Fermi/LAT errorbox, therefore we exclude their association with GRB 220627A. Within the error box of the uncatalogued X-ray Source 3 discovered by Swift/XRT through ToO observations (Evans, GCN 32284), we detect a new transient candidate at the following coordinates: RA (J2000) = 13:25:28.49 (201.36872d) Dec (J2000) = -32:25:33.31 (-32.42592d) calibrated against Gaia DR2, with a positional uncertainty of 0.1" in each coordinate. The same object is detected in a further 2x300s observations ~1 hour later. The source is detected with an AB magnitude of q = 21.25 +/- 0.09 in the first exposure. We detect no source at the transient location in an archival image of the same field down to a 3-sigma limiting magnitude of q > 21.71. We suggest this may be the afterglow of GRB 220627A. Further follow-up is encouraged. MeerLICHT is built and run by a consortium consisting of Radboud University, University of Cape Town, the South African Astronomical Observatory, the University of Oxford, the University of Manchester and the University of Amsterdam.