@Article{ANTARESCollaborationAlbert_etal2017,
author="ANTARES Collaboration (Albert, A. et al
and Barrios-Marti, J.
and Hernandez-Rey, J. J.
and Illuminati, G.
and Lotze, M.
and T{\"o}nnis, C.
and Zornoza, J. D.
and Zu{\~{n}}iga, J.",
title="Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope",
journal="Physics Letters B",
year="2017",
publisher="Elsevier Science Bv",
volume="769",
pages="249--254",
optkeywords="Dark matter; WIMP; Indirect detection; Neutrino telescope; Galactic Centre; ANTARES",
abstract="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.",
optnote="WOS:000402342500040",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3160), last updated on Mon, 19 Aug 2019 06:52:24 +0000",
issn="0370-2693",
doi="10.1016/j.physletb.2017.03.063",
opturl="http://arxiv.org/abs/1612.04595",
opturl="https://doi.org/10.1016/j.physletb.2017.03.063",
archivePrefix="arXiv",
eprint="1612.04595",
language="English"
}