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dc.contributor.authorAcero, F.
dc.contributor.authorAharonian, F.
dc.contributor.authorAkhperjanian, A.
dc.contributor.authorAnton, G.
dc.contributor.authorBarres de Almeida, U.
dc.contributor.authorBazer-Bachi, A.
dc.contributor.authorBecherini, Y.
dc.contributor.authorBehera, B.
dc.contributor.authorBernlöhr, K.
dc.contributor.authorBochow, A.
dc.contributor.authorBoisson, C.
dc.contributor.authorBolmont, J.
dc.contributor.authorBorrel, V.
dc.contributor.authorBrucker, J.
dc.contributor.authorBrun, F.
dc.contributor.authorBrun, P.
dc.contributor.authorBüHLER, R.
dc.contributor.authorBulik, T.
dc.contributor.authorBüsching, I.
dc.contributor.authorBoutelier, T.
dc.contributor.authorChadwick, P.
dc.contributor.authorCharbonnier, A.
dc.contributor.authorChaves, R.
dc.contributor.authorCheesebrough, A.
dc.contributor.authorChounet, L.
dc.contributor.authorClapson, A.
dc.contributor.authorCoignet, G.
dc.contributor.authorDalton, M.
dc.contributor.authorDaniel, M.
dc.contributor.authorDavids, I.
dc.contributor.authorDegrange, B.
dc.contributor.authorDeil, C.
dc.contributor.authorDickinson, H.
dc.contributor.authorDjannati-Ataï, A.
dc.contributor.authorDomainko, W.
dc.contributor.authorDrury, L.
dc.contributor.authorDubois, F.
dc.contributor.authorDubus, G.
dc.contributor.authorDyks, J.
dc.contributor.authorDyrda, M.
dc.contributor.authorEgberts, K.
dc.contributor.authorEmmanoulopoulos, D.
dc.contributor.authorEspigat, P.
dc.contributor.authorFarnier, C.
dc.contributor.authorFegan, S.
dc.contributor.authorFeinstein, F.
dc.contributor.authorFiasson, A.
dc.contributor.authorFörster, A.
dc.contributor.authorFontaine, G.
dc.contributor.authorFüßling, M.
dc.contributor.authorGabici, S.
dc.contributor.authorGallant, Y.
dc.contributor.authorGerard, L.
dc.contributor.authorGerbig, D.
dc.contributor.authorGiebels, B.
dc.contributor.authorGlicenstein, J.
dc.contributor.authorGlück, B.
dc.contributor.authorGoret, P.
dc.contributor.authorGöring, D.
dc.contributor.authorHäuser, D.
dc.contributor.authorHauser, M.
dc.contributor.authorHeinz, S.
dc.contributor.authorHeinzelmann, G.
dc.contributor.authorHenri, G.
dc.contributor.authorHermann, G.
dc.contributor.authorHinten, J.
dc.contributor.authorHoffmann, A.
dc.contributor.authorHofmann, W.
dc.contributor.authorHofverberg, P.
dc.contributor.authorHoppe, P.
dc.contributor.authorHorns, D.
dc.contributor.authorJacholkowska, A.
dc.contributor.authorDe Jager, O.
dc.contributor.authorJahn, C.
dc.contributor.authorJung, I.
dc.contributor.authorKatarzynski, K.
dc.contributor.authorKatz, U.
dc.contributor.authorKaufmann, S.
dc.contributor.authorKerschhaggl, M.
dc.contributor.authorKhangulyan, D.
dc.contributor.authorKhélifi, B.
dc.contributor.authorKeogh, D.
dc.contributor.authorKlochkov, D.
dc.contributor.authorKluzniak, W.
dc.contributor.authorKneiske, T.
dc.contributor.authorKomin, N.
dc.contributor.authorKosack, K.
dc.contributor.authorKossakowski, R.
dc.contributor.authorLamanna, G.
dc.contributor.authorLenain, J.
dc.contributor.authorLohse, T.
dc.contributor.authorMarandon, V.
dc.contributor.authorMartineau-Huynh, O.
dc.contributor.authorMarcowith, A.
dc.contributor.authorMasbou, J.
dc.contributor.authorMaurin, D.
dc.contributor.authorMcComb, T.
dc.contributor.authorMedina, C.
dc.contributor.authorMehault, J.
dc.contributor.authorModerski, R.
dc.contributor.authorMoulin, E.
dc.contributor.authorNaumann-Godo, M.
dc.contributor.authorde Naurois, M.
dc.contributor.authorNedbal, D.
dc.contributor.authorNekrassov, D.
dc.contributor.authorNicholas, B.
dc.contributor.authorNiemiec, J.
dc.contributor.authorNolan, S.
dc.contributor.authorOhm, S.
dc.contributor.authorOlive, J.
dc.contributor.authorde Oña Wilhelmi, E.
dc.contributor.authorOrford, K.
dc.contributor.authorOstrowski, M.
dc.contributor.authorPanter, M.
dc.contributor.authorPaz Arribas, M.
dc.contributor.authorPedaletti, G.
dc.contributor.authorPelletier, G.
dc.contributor.authorPetrucci, P.
dc.contributor.authorPita, S.
dc.contributor.authorPühlhofer, G.
dc.contributor.authorPunch, M.
dc.contributor.authorOuirrenbach, A.
dc.contributor.authorRaubenheimer, B.
dc.contributor.authorRaue, M.
dc.contributor.authorRayner, S.
dc.contributor.authorReimer, O.
dc.contributor.authorRenaud, M.
dc.contributor.authorRieger, F.
dc.contributor.authorRipken, J.
dc.contributor.authorRob, L.
dc.contributor.authorRosier Lees, S.
dc.contributor.authorRowell, G.
dc.contributor.authorRudak, B.
dc.contributor.authorRulten, C.
dc.contributor.authorRuppel, J.
dc.contributor.authorSahakian, V.
dc.contributor.authorSantangelo, A.
dc.contributor.authorSchlickeiser, R.
dc.contributor.authorSchöck, F.
dc.contributor.authorSchwanke, U.
dc.contributor.authorSchwarzburg, S.
dc.contributor.authorSchwemmer, S.
dc.contributor.authorShalchi, A.
dc.contributor.authorSikora, M.
dc.contributor.authorSkilton, J.
dc.contributor.authorSol, H.
dc.contributor.authorStawarz, L.
dc.contributor.authorSteenkamp, R.
dc.contributor.authorStegmann, C.
dc.contributor.authorStinzing, F.
dc.contributor.authorSuperina, G.
dc.contributor.authorSzostek, A.
dc.contributor.authorTam, P.
dc.contributor.authorTavernet, J.
dc.contributor.authorTerrier, R.
dc.contributor.authorTibolla, Omar
dc.contributor.authorTluczykont, M.
dc.contributor.authorvan Eldik, C.
dc.contributor.authorVasileiadis, G.
dc.contributor.authorVenter, C.
dc.contributor.authorVenter, L.
dc.contributor.authorVialle, J.
dc.contributor.authorVincent, P.
dc.contributor.authorVivier, M.
dc.contributor.authorVolk, H.
dc.contributor.authorVolpe, F.
dc.contributor.authorWagner, S.
dc.contributor.authorWard, M.
dc.contributor.authorZdziarski, A.
dc.contributor.authorZech, A.
dc.date.accessioned2017-01-30T11:22:13Z
dc.date.available2017-01-30T11:22:13Z
dc.date.created2014-11-19T01:13:31Z
dc.date.issued2009
dc.identifier.citationAcero, F. and Aharonian, F. and Akhperjanian, A. and Anton, G. and Barres de Almeida, U. and Bazer-Bachi, A. and Becherini, Y. et al. 2009. Detection of Gamma Rays from a Starburst Galaxy. Science. 326 (5956): pp. 1080-1082.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/10999
dc.description.abstract

Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of ~1015 electron volts. We report the detection of gamma rays---tracers of such cosmic rays---from the starburst galaxy NGC 253 using the High Energy Stereoscopic System (H.E.S.S.) array of imaging atmospheric Cherenkov telescopes. The gamma-ray flux above 220 billion electron volts is F = (5.5 ± 1.0stat ± 2.8sys) × 10-13 cm-2 s-1, implying a cosmic-ray density about three orders of magnitude larger than that in the center of the Milky Way. The fraction of cosmic-ray energy channeled into gamma rays in this starburst environment is five times as large as that in our Galaxy.

dc.publisherThe American Association for the Advancement of Science
dc.titleDetection of Gamma Rays from a Starburst Galaxy
dc.typeJournal Article
dcterms.source.volume326
dcterms.source.number5956
dcterms.source.startPage1080
dcterms.source.endPage1082
dcterms.source.issn0036-8075
dcterms.source.titleScience
curtin.accessStatusFulltext not available


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