Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope. (arXiv:1612.04595v3 [astro-ph.HE] UPDATED)

Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope. (arXiv:1612.04595v3 [astro-ph.HE] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Albert_A/0/1/0/all/0/1">A. Albert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Andre_M/0/1/0/all/0/1">M. André</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anghinolfi_M/0/1/0/all/0/1">M. Anghinolfi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anton_G/0/1/0/all/0/1">G. Anton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ardid_M/0/1/0/all/0/1">M. Ardid</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aubert_J/0/1/0/all/0/1">J.-J. Aubert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Avgitas_T/0/1/0/all/0/1">T. Avgitas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baret_B/0/1/0/all/0/1">B. Baret</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barrios_Marti_J/0/1/0/all/0/1">J. Barrios-Martí</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Basa_S/0/1/0/all/0/1">S. Basa</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertin_V/0/1/0/all/0/1">V. Bertin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Biagi_S/0/1/0/all/0/1">S. Biagi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bormuth_R/0/1/0/all/0/1">R. Bormuth</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bourret_S/0/1/0/all/0/1">S. Bourret</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bouwhuis_M/0/1/0/all/0/1">M.C. Bouwhuis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bruijn_R/0/1/0/all/0/1">R. Bruijn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brunner_J/0/1/0/all/0/1">J. Brunner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Busto_J/0/1/0/all/0/1">J. Busto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Capone_A/0/1/0/all/0/1">A. Capone</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Caramete_L/0/1/0/all/0/1">L. Caramete</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carr_J/0/1/0/all/0/1">J. Carr</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Celli_S/0/1/0/all/0/1">S. Celli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chiarusi_T/0/1/0/all/0/1">T. Chiarusi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Circella_M/0/1/0/all/0/1">M. Circella</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coelho_J/0/1/0/all/0/1">J.A.B. Coelho</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coleiro_A/0/1/0/all/0/1">A. Coleiro</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coniglione_R/0/1/0/all/0/1">R. Coniglione</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Costantini_H/0/1/0/all/0/1">H. Costantini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coyle_P/0/1/0/all/0/1">P. Coyle</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Creusot_A/0/1/0/all/0/1">A. Creusot</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Deschamps_A/0/1/0/all/0/1">A. Deschamps</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bonis_G/0/1/0/all/0/1">G. De Bonis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Distefano_C/0/1/0/all/0/1">C. Distefano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Donzaud_I/0/1/0/all/0/1">I. Di Palma Donzaud</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Dornic_D/0/1/0/all/0/1">D. Dornic</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Drouhin_D/0/1/0/all/0/1">D. Drouhin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Eberl_T/0/1/0/all/0/1">T. Eberl</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bojaddaini_I/0/1/0/all/0/1">I. El Bojaddaini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Elsasser_D/0/1/0/all/0/1">D. Elsässer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Enzenhofer_A/0/1/0/all/0/1">A. Enzenhöfer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Felis_I/0/1/0/all/0/1">I. Felis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Fusco_L/0/1/0/all/0/1">L.A. Fusco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Galata_S/0/1/0/all/0/1">S. Galatà</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gay_P/0/1/0/all/0/1">P. Gay</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Geisselsoder_S/0/1/0/all/0/1">S. Geißelsöder</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Geyer_K/0/1/0/all/0/1">K. Geyer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Giordano_V/0/1/0/all/0/1">V. Giordano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gleixner_A/0/1/0/all/0/1">A. Gleixner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Glotin_H/0/1/0/all/0/1">H. Glotin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gozzini_R/0/1/0/all/0/1">R. Gozzini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gregoire_T/0/1/0/all/0/1">T. Grégoire</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gracia_Ruiz_R/0/1/0/all/0/1">R. Gracia-Ruiz</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Graf_K/0/1/0/all/0/1">K. Graf</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hallmann_S/0/1/0/all/0/1">S. Hallmann</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Haren_H/0/1/0/all/0/1">H. van Haren</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Heijboer_A/0/1/0/all/0/1">A.J. Heijboer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hello_Y/0/1/0/all/0/1">Y. Hello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hernandez_Rey_J/0/1/0/all/0/1">J.J. Hernández-Rey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hossl_J/0/1/0/all/0/1">J. Hößl</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hofestadt_J/0/1/0/all/0/1">J. Hofestädt</a>, et al. (68 additional authors not shown)

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, $rm WIMP + WIMP to b bar b, W^+
W^-, tau^+ tau^-, mu^{+} mu^{-}$ and $nu bar{nu}$, with WIMP masses
ranging from 50 $frac{text{GeV}}{text{c}^2}$ to 100
$frac{text{TeV}}{text{c}^2}$, were considered. No excess over the expected
background was found, and limits on the thermally averaged annihilation
cross–section were set.

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