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Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data

  • (The Fermi-LAT Collaboration)
  • German Electron Synchrotron
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stockholm University
  • Oskar Klein Centre
  • University of California at Santa Cruz
  • University of Pisa
  • National Institute for Nuclear Physics
  • University of Trieste
  • University of Padua
  • University of Wisconsin-Madison
  • University of Turin
  • NASA Goddard Space Flight Center
  • LUPM-UMR 5299, CNRS, Université Montpellier
  • Laboratoire Leprince-Ringuet
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • University of Perugia
  • George Mason University
  • Naval Research Laboratory
  • Italian Space Agency
  • Osservatorio Astronomico Roma
  • Wallenberg Academy Fellow
  • National Institute for Astrophysics
  • University of Bologna
  • University of Udine
  • Pegaso Telematic University
  • Polytechnic University of Bari
  • Fermi National Accelerator Laboratory
  • Hiroshima University

Research output: Contribution to journalArticlepeer-review

1102 Scopus citations

Abstract

The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass 100 GeV annihilating via quark and τ-lepton channels.

Original languageEnglish
Article number231301
JournalPhysical Review Letters
Volume115
Issue number23
DOIs
StatePublished - Nov 30 2015

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