TITLE: GCN CIRCULAR NUMBER: 36307 SUBJECT: S240422ed: BlackGEM/MeerLICHT transient detection AT2024hgl/MLTJ080628.10-250116.4 DATE: 24/04/25 17:01:30 GMT FROM: Paul Groot at Radboud University Nijmegen P.J. Groot (Radboud, UCT, SAAO), H. Tranin (Barcelona), H. Wichern (DTU), G. Leloudas (DTU), F. Stoppa (Radboud), I. Arcavi (Tel Aviv), S. Bloemen (Radboud), P.M. Vreeswijk (Radboud), D. Pieterse (Radboud) report on behalf of the BlackGEM/MeerLICHT Consortium: Following the LVK Alert S240422ed the 0.6m BlackGEM/MeerLICHT telescope array located at the ESO La Silla, Chile and SAAO Sutherland, South Africa observatories observed the error box with the ML1/BG2/BG4 telescopes using a predefined sky-grid tiling that covers the accessible part of the error region using the ranked-tiling method as outlined in Ghosh et al. (2016). Observations were obtained in the q band, spanning 440-720nm, using a 2x10-tile strategy. Starting with the highest probability tiles a set of 10-tiles was observed in the q-band filter using 60s exposures each, which was repeated directly after the first 10 tiles were observed. Subsequently tiles 11-20 were observed in the same two-visit manner, etc. Observations on the Updated error region of S240422ed (Biscoveanu et al., GCN Circular 36240) were repeated on the nights of 2024-04-23 and 2024-04-24 following the same tiling pattern. Transient candidates were extracted using the BlackBOX/ZOGY pipeline, where astrophotometric calibrations are performed using Gaia DR3 photometry and astrometry. Possible asteroids are filtered using the daily-updated lists of known asteroids from the Minor Planet Center. All coordinates are given in the ICRS, epoch J2016.0 astrometric frame and magnitudes quoted are on the AB system. Next to the MeerLICHT/BlackGEM detection of AT 2024hfx (Smith et al., GCN36303; Groot et al., GCN36304) we find one more candidate that cannot be ruled out as the counterpart to S240422ed: Name RA (ICRS) Dec(ICRS) Filter AB-Mag Date-UT MLTJ080628.10-250116.4 121.61711 -25.02119 q 19.92+/-0.16 2024-04-24 17:32:29 "" "" "" q 19.70+/-0.15 2024-04-24 17:45:43 The candidate was reported to the Transient Name Server as AT2024hgl. The last non-detection at this position with MeerLICHT was obtained on 2022-01-28 and is therefore not constraining. Inspection of the public ATLAS archive shows no recent brightening or flaring at the source location. The BlackGEM/MeerLICHT telescopes are designed, installed and operated by a consortium of the following universities and institutions: Radboud University, Netherlands Research School for Astronomy NOVA, KU Leuven, Armagh Observatory and Planetarium, Hebrew University of Jerusalem, South African Astronomical Observatory, Technical University of Denmark, Tel Aviv University, Texas Tech University, University of Amsterdam, University of Barcelona, University of California at Davis, University of Cape Town, University of Durham, University of Hamburg, University of Manchester, University of Oxford, University of Potsdam, University of Valparaiso, University of Warwick, Weizmann Institute References: Ghosh et al., 2016, A&A 592, 82