2011
DOI: 10.1103/physrevlett.107.241302
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Constraining Dark Matter Models from a Combined Analysis of Milky Way Satellites with the Fermi Large Area Telescope

Abstract: Satellite galaxies of the Milky Way are among the most promising targets for dark matter searches in gamma rays. We present a search for dark matter consisting of weakly interacting massive particles, applying a joint likelihood analysis to 10 satellite galaxies with 24 months of data of the Fermi Large Area Telescope. No dark matter signal is detected. Including the uncertainty in the dark matter distribution, robust upper limits are placed on dark matter annihilation cross sections. The 95% confidence level … Show more

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Cited by 507 publications
(533 citation statements)
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“…from γ ray searches in the Milky Way satellite galaxies by Fermi [73] or antiproton searches by PAMELA [74,75] and BESS-Polar II [76,77], are in general weaker than those from the continuum γs studied previously. To illustrate that in the GNMSSM, the Fermi line can be explained while all direct and indirect detection constraints are satisfied, we provide an explicit example in the next section.…”
Section: Jhep01(2013)124mentioning
confidence: 90%
“…from γ ray searches in the Milky Way satellite galaxies by Fermi [73] or antiproton searches by PAMELA [74,75] and BESS-Polar II [76,77], are in general weaker than those from the continuum γs studied previously. To illustrate that in the GNMSSM, the Fermi line can be explained while all direct and indirect detection constraints are satisfied, we provide an explicit example in the next section.…”
Section: Jhep01(2013)124mentioning
confidence: 90%
“…The strongest constraints for light DM 9 annihilating into bb or τ + τ − is provided by the measurements of the gamma-ray flux from Dwarf Spheroidal Galaxies by the Fermi-LAT satellite, ruling out the canonical crosssection [41,42]:…”
Section: Jhep11(2014)016mentioning
confidence: 99%
“…For m S 3 < 20 GeV, the predicted annihilation rate for the τ + τ − final-state is in some tension with upper limits inferred from searches for DM signals in diffuse gamma-ray data from the Fermi Large Area Telescope observations of dwarf spheroidal satellite galaxies of the Milky Way [62][63][64].…”
Section: Effective Dm-lepton Interactionsmentioning
confidence: 99%