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Bachetti, M. Burgay, M. Fiori, M. Ge, M. Orlandini, M. Perri, M. Pilia, M. Tavani, M. Trudu, P. Casella, P. Ochener, R. Burenin, S. Jia, S.L. Xiong, S.N. Zhang, S. Zheltoukhov, V. Gajjar, V.R. Marthi, V. Savchenko, X. Li","submitted_at":"2023-05-29T21:32:55Z","abstract_excerpt":"Aims. Fast Radio Bursts are bright radio transients whose origin has not yet explained. The search for a multi-wavelength counterpart of those events can put a tight constrain on the emission mechanism and the progenitor source. Methods. We conducted a multi-wavelength observational campaign on FRB 20180916B between October 2020 and August 2021 during eight activity cycles of the source. Observations were led in the radio band by the SRT both at 336 MHz and 1547 MHz and the uGMRT at 400 MHz. 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