%0 Journal Article
%9 ACL : Articles dans des revues avec comité de lecture répertoriées par l'AERES
%A Albert, A.
%A Andre, M.
%A Anghinolfi, M.
%A Anton, G.
%A Ardid, M.
%A Aubert, J. J.
%A Avgitas, T.
%A Baret, B.
%A Barrios-Marti, J.
%A Basa, S.
%A Bertin, V.
%A Biagi, S.
%A Bormuth, R.
%A Bourret, S.
%A Bouwhuis, M. C.
%A Bruijn, R.
%A Brunner, J.
%A Busto, J.
%A Capone, A.
%A Caramete, L.
%A Carr, J.
%A Celli, S.
%A Chiarusi, T.
%A Circella, M.
%A Coelho, J. A. B.
%A Coleiro, A.
%A Coniglione, R.
%A Costantini, H.
%A Coyle, P.
%A Creusot, A.
%A Deschamps, A.
%A De Bonis, G.
%A Distefano, C.
%A Di Palma, I.
%A Donzaud, C.
%A Dornic, D.
%A Drouhin, D.
%A Eberl, T.
%A El Bojaddaini, I.
%A Elsasser, D.
%A Enzenhofer, A.
%A Felis, I.
%A Fusco, L. A.
%A Galata, S.
%A Gay, P.
%A Geisselsoder, S.
%A Geyer, K.
%A Giordano, V.
%A Gleixner, A.
%A Glotin, H.
%A Gregoire, T.
%A Ruiz, R. G.
%A Graf, K.
%A Hallmann, S.
%A Van Haren, H.
%A Heijboer, A. J.
%A Hello, Yann
%A et al.
%T Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope [+ Erratum in Physical Letters : B. 2019, vol. 796, pp. 253-255]
%D 2017
%L fdi:010070199
%G ENG
%J Physics Letters B
%@ 0370-2693
%K Dark matter ; WIMP ; Indirect detection ; Neutrino telescope ; Galactic ; Centre ; ANTARES
%M ISI:000402342500040
%P 249-254 [+ Erratum in Physical Letters : B. 2019, vol. 796, p 253-255]
%R 10.1016/j.physletb.2017.03.063
%U https://www.documentation.ird.fr/hor/fdi:010070199
%> https://horizon.documentation.ird.fr/exl-doc/pleins_textes/divers17-06/010070199.pdf
%V 769
%W Horizon (IRD)
%X Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, WIMP + WIMP -> b (b) over bar, W+W-, tau(+)tau(-), mu(+)mu(-) and v (v) over bar, with WIMP masses ranging from 50 2 GeV/C-2 to 100 Tev/C-2, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross-section were set.
%$ 060 ; 020