%0 Conference Proceedings
%T Detecting supersymmetric dark matter in M31 with CELESTE ?
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%+ Laboratoire de Physique Mathématique et Théorique (PMT)
%+ Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH)
%A Nuss, E.
%A Moultaka, G.
%A Falvard, Alain
%A Giraud, E.
%A Jacholkowska, A.
%A Jedamzik, K.
%A Lavalle, J.
%A Piron, F.
%A Sapinski, M.
%A Salati, P.
%A Taillet, Richard
%Z Latex, 5 pages, 3 figures, to appear in the proceedings of the French Astrophysical Society, 2002 - GAM
%< avec comité de lecture
%( Société Française d'Astronomie et d'Astrophysique Scientific Higlights 2002
%B The SN factory Consortium - SF2A-2002 - Semaine de l'Astrophysique Française
%C Paris, France
%Y F. Combes and D. Barret
%I EDP Sciences
%3 Conference Series
%8 2002-06-24
%D 2002
%Z astro-ph/0212560
%Z Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]Conference papers
%X It is widely believed that dark matter exists within galaxies and clusters of galaxies. Under the assumption that this dark matter is composed of the lightest, stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indirect detection via observations of a diffuse gamma-ray signal due to neutralino annihilation within M31 is examined.
%G English
%L in2p3-00087404
%U https://hal.in2p3.fr/in2p3-00087404
%~ IN2P3
%~ UNIV-SAVOIE
%~ UGA
%~ LPTA
%~ CNRS
%~ UNIV-MONTP2
%~ LAPTH
%~ UNIV-MONTPELLIER
%~ USMB-COMUE
%~ UM1-UM2