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On October 1, 2019, the IceCube Collaboration detected a muon track neutrinowith high probability of being of astrophysical origin, IC191001A. After a fewhours, the tidal disruption event (TDE) AT2019dsg, observed by the ZwickyTransient Facility (ZTF), was indicated as the most likely counterpart of theIceCube track. More recently, the follow-up campaign of the IceCube alerts byZTF suggested a second TDE, AT2019fdr, as a promising counterpart of anotherIceCube muon track candidate, IC200530A, detected on May 30, 2020. These arethe second and third associations between astrophysical sources and high-energyneutrinos after the compelling identification of the blazar TXS 0506+056. Here,the search for ANTARES neutrinos from the directions of AT2019dsg and AT2019fdrusing a time-integrated approach is presented. As no significant evidence forspace clustering is found in the ANTARES data, upper limits on the one-flavourneutrino flux and fluence are set.

Search for neutrinos from the tidal disruption events AT2019dsg and AT2019fdr with the ANTARES telescope