tokens: Acknowledgments TS acknowledges financial support from the Japan Society for the Promotion of Science (JSPS) under grant numbers JSPS23103002, JSPS24253004 and JSPS26247023. NK is supported by Grant-in-Aid for JSPS Fellows. The MOA project is supported by JSPS grants JSPS25103508 and JSPS23340064 and by the Royal Society of New Zealand Marsden Grant MAU1104. NJR acknowledges the contribution of NeSI high-performance computing facilities to the results of this research. New Zealands national facilities are provided by the NZ eScience Infrastructure and funded jointly by NeSIs collaborator institutions and through the Ministry of Business, Innovation Employments Research Infrastructure programme ( https://www.nesi.org.nz ). The OGLE team thanks Prof. M. Kubiak and G. Pietrzyski, former members of the OGLE team, for their contribution to the collection of the OGLE photometric data over the past years. The OGLE project has received funding from the National Science Centre, Poland, grant MAESTRO 2014/14/A/ST9/00121 to AU. The Danish 1.54m telescope is operated based on a grant from the Danish Natural Science Foundation (FNU). The MiNDSTEp monitoring campaign is powered by ARTEMiS (Automated Terrestrial Exoplanet Microlensing Search; Dominik etal. 2008 ). This publication was made possible by NPRP grant nos. X-019-1-006 and 09-467-1-078 from the Qatar National Research Fund (a member of Qatar Foundation). KH acknowledges support from STFC grant ST/M001296/1. GD acknowledges Regione Campania for support from POR-FSE Campania 2014-2020. TCH acknowledges support from the Korea Research Council of Fundamental Science Technology (KRCF) via the KRCF Young Scientist Research Fellowship Programme and for financial support from KASI travel grant number 2014-1-400-06. JS acknowledges support from the Communaut franaise de Belgique - Actions de recherche concertes - Acadmie Wallonie-Europe. This work has made extensive use of the ADS service, for which we are thankful. This work makes use of observations from the LCOGT network, which includes three SUPAscopes owned by the University of St Andrews. The RoboNET programme is an LCOGT Key Project using time allocations from the University of St Andrews, LCOGT and the University of Heidelberg together with time on the Liverpool Telescope through the Science and Technology Facilities Council (STFC), UK. This research has made use of the LCOGT Archive, which is operated by the California Institute of Technology, under contract with the Las Cumbres Observatory. The authors thank Matthew Penny for his comments on this manuscript.
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