Albert, A.Andre, M.Anghinolfi, M.Anton, G.Ardid, MiguelAubert, J.-J.Aublin, J.Avgitas, T.Baret, B.Barrios-Marti, J.Basa, S.Belhorma, B.Bertin, V.Biagi, S.Bormuth, R.MartÃnez Mora, Juan Antonio2021-01-122021-01-122019-06-21https://riunet.upv.es/handle/10251/158690[EN] The ANTARES neutrino telescope has an energy threshold of a few tens of GeV. This allows to study the phenomenon of atmospheric muon neutrino disappearance due to neutrino oscillations. In a similar way, constraints on the 3+1 neutrino model, which foresees the existence of one sterile neutrino, can be inferred. Using data collected by the ANTARES neutrino telescope from 2007 to 2016, a new measurement of Dm2 32 and 023 has been performed - which is consistent with world best- t values - and constraints on the 3+1 neutrino model have been derived.Reconocimiento (by)Neutrino detectors and telescopes (experiments)OscillationFISICA APLICADAMeasuring the atmospheric neutrino oscillation parameters and constraining the 3+1 neutrino model with ten years of ANTARES dataArtÃculo10.1007/JHEP06(2019)113Abierto1029-8479