%0 Journal Article
%T HESS Observations of the Galactic Center Region and Their Possible Dark Matter Interpretation
%+ Centre d'étude spatiale des rayonnements (CESR)
%+ Laboratoire Univers et Théories (LUTH (UMR_8102))
%+ Laboratoire Leprince-Ringuet (LLR)
%+ APC - Astrophysique des Hautes Energies (APC - AHE)
%+ AstroParticule et Cosmologie (APC (UMR_7164))
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%+ Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA)
%+ Laboratoire d'Astrophysique de Grenoble (LAOG)
%+ Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE)
%A Aharonian, F.
%A Akhperjanian, A. G.
%A Bazer-Bachi, A.R.
%A Beilicke, M.
%A Benbow, W.
%A Berge, D.
%A Bernlöhr, K.
%A Boisson, C.
%A Bolz, O.
%A Borrel, V.
%A Braun, I.
%A Breitling, F.
%A Brown, A. M.
%A Bühler, R.
%A Büsching, I.
%A Carrigan, S.
%A Chadwick, P. M.
%A Chounet, L.-M.
%A Cornils, R.
%A Costamante, L.
%A Degrange, B.
%A Dickinson, H. J.
%A Djannati-Ataï, A.
%A Drury, L. O.'C.
%A Dubus, G.
%A Egberts, K.
%A Emmanoulopoulos, D.
%A Espigat, P.
%A Feinstein, F.
%A Ferrero, E.
%A Fiasson, A.
%A Fontaine, G.
%A Funk, Seb.
%A Funk, S.
%A Gallant, Y.A.
%A Giebels, B.
%A Glicenstein, J. F.
%A Goret, P.
%A Hadjichristidis, C.
%A Hauser, D.
%A Hauser, M.
%A Heinzelmann, G.
%A Henri, G.
%A Hermann, G.
%A Hinton, J. A.
%A Hofmann, W.
%A Holleran, M.
%A Horns, D.
%A Jacholkowska, A.
%A de Jager, O. C.
%A Khélifi, B.
%A Komin, Nu.
%A Konopelko, A.
%A Kosack, K.
%A Latham, I. J.
%A Le Gallou, R.
%A Lemière, A.
%A Lemoine-Goumard, M.
%A Lohse, T.
%A Martin, J.M.
%A Martineau-Huynh, O.
%A Marcowith, A.
%A Masterson, C.
%A Mccomb, T. J. L.
%A de Naurois, M.
%A Nedbal, D.
%A Nolan, S. J.
%A Noutsos, A.
%A Orford, K. J.
%A Osborne, J. L.
%A Ouchrif, M.
%A Panter, M.
%A Pelletier, G.
%A Pita, S.
%A Pühlhofer, G.
%A Punch, M.
%A Raubenheimer, B. C.
%A Raue, M.
%A Rayner, S. M.
%A Reimer, A.
%A Reimer, O.
%A Ripken, J.
%A Rob, L.
%A Rolland, L.
%A Rowell, G.
%A Sahakian, V.
%A Saugé, L.
%A Schlenker, S.
%A Schlickeiser, R.
%A Schwanke, U.
%A Sol, H.
%A Spangler, D.
%A Spanier, F.
%A Steenkamp, R.
%A Stegmann, C.
%A Superina, G.
%A Tavernet, J.-P.
%A Terrier, R.
%A Théoret, C.G.
%A Tluczykont, M.
%A van Eldik, C.
%A Vasileiadis, G.
%A Venter, C.
%A Vincent, P.
%A Völk, H. J.
%A Wagner, S. J.
%A Ward, M.
%Z 5 pages, 2 figures, published in Physical Review Letters Correct some references The accepted version set on astro-ph was slightly too long for publication. This is a slightly shorter version
%< avec comité de lecture
%Z APC-06-116
%@ 0031-9007
%J Physical Review Letters
%I American Physical Society
%V 97
%P 221102
%8 2006
%D 2006
%Z astro-ph/0610509
%Z 2006PhRvL..97v1102A
%R 10.1103/PhysRevLett.97.221102
%Z 98.70.Rz, 95.35.+d, 95.85.Pw, 98.35.Jk
%Z Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]Journal articles
%X The detection of gamma rays from the source HESS J1745-290 in the Galactic Center (GC) region with the High Energy Spectroscopic System (HESS) array of Cherenkov telescopes in 2004 is presented. After subtraction of the diffuse gamma-ray emission from the GC ridge, the source is compatible with a point source with spatial extent less than 1.2[prime](stat) (95% C.L.). The measured energy spectrum above 160 GeV is compatible with a power law with photon index of 2.25±0.04(stat)±0.10(syst) and no significant flux variation is detected. It is finally found that the bulk of the very high energy emission must have non-dark-matter origin.
%G English
%Z HESS
%L in2p3-00137679
%U https://hal.in2p3.fr/in2p3-00137679
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