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dc.contributor.authorAbramowski, A.
dc.contributor.authorBüsching, I.
dc.contributor.authorDe Jager, O.C.
dc.contributor.authorVenter, C.
dc.contributor.authorVorster, M.
dc.contributor.authorH.E.S.S. Collaboration
dc.identifier.citationAbramowski, A. et al. 2011. H.E.S.S. constraints on dark matter annihilations towards the Sculptor and Carina dwarf galaxies. Astroparticle physics, 34(8):608-616. []en_US
dc.identifier.issn1873-2852 (Online)
dc.description.abstractThe Sculptor and Carina dwarf spheroidal galaxies were observed with the H.E.S.S. Cherenkov telescope array between January 2008 and December 2009. The data sets consist of a total of 11.8 h and 14.8 h of high quality data, respectively. No gamma-ray signal was detected at the nominal positions of these galaxies above 220 GeV and 320 GeV, respectively. Upper limits on the gamma-ray fluxes at 95% CL assuming two forms for the spectral energy distribution (a power law shape and one derived from dark matter annihilation) are obtained at the level of 10-13-10-12 cm-2 s-1 in the TeV range. Constraints on the velocity weighted dark matter particle annihilation cross section for both Sculptor and Carina dwarf galaxies range from σʋ~ 10-21 cm3 s-1 down to σʋ i ~ 10-22 cm3 s-1 depending on the dark matter halo model used. Possible enhancements of the gamma-ray flux are studied: the Sommerfeld effect, which is found to exclude some dark matter particle masses, the internal Bremsstrahlung and clumps in the dark-matter halo distributions.en_US
dc.subjectGamma-rays: observationsen_US
dc.subjectdark matteren_US
dc.subjectSommerfeld enhancementen_US
dc.subjectInternal Bremsstrahlungen_US
dc.subjectDwarf spheroidal galaxy
dc.titleH.E.S.S. constraints on dark matter annihilations towards the Sculptor and Carina dwarf galaxiesen_US
dc.contributor.researchID12006653 - Venter, Christo
dc.contributor.researchID13235176 - Büsching, Ingo
dc.contributor.researchID10065857 - De Jager, Ocker Cornelis
dc.contributor.researchID12792322 - Vorster, Michael Johannes

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