{"refrec":{"BRefID":282233,"RR":"<b>Adrian-Martinez, S.; van Haren, H.</b> (2016). Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope. <i>Phys. Lett. B 759</i>: 69–74. <a href=\"https://dx.doi.org/10.1016/j.physletb.2016.05.019\" target=\"_blank\">https://dx.doi.org/10.1016/j.physletb.2016.05.019</a>","BEntID":274252,"PublicFlag":1,"CheckedFlag":0,"wosflag":1,"vabbflag":1,"RefStringPartII":". <i>Phys. Lett. B 759</i>: 69–74. <a href=\"https://dx.doi.org/10.1016/j.physletb.2016.05.019\" target=\"_blank\">https://dx.doi.org/10.1016/j.physletb.2016.05.019</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Adrian-Martinez, S.; van Haren, H.","OrigTitleTranslFlag":0,"Authorstringtrunc":"Adrian-Martinez, S.; van Haren, H.","Englishabstract":"A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. 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