Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data
Journal Article
·
· Phys.Rev.Lett.
more »
- DESY
- Stanford U., HEPL; KIPAC, Menlo Park; Stanford U., Phys. Dept.
- Stockholm U., OKC
- UC, Santa Cruz
- INFN, Pisa
- INFN, Trieste; Trieste U.
- INFN, Padua; Padua U.
- Chicago U., KICP
- INFN, Bari
- INFN, Turin; Turin U.
- NASA, Goddard
- U. Montpellier 2, LUPM
- Ecole Polytechnique
- Stanford U., HEPL; KIPAC, Menlo Park; Stanford U., Phys. Dept.; CIFS, Turin
- Brera Observ.
- INFN, Perugia; Perugia U.
- George Washington U.
- Padua U.
- INFN, Rome2; INFN, Perugia; Rome Observ.
- Stockholm U.; Stockholm U., OKC
- Stockholm U., OKC; INFN, Turin; Turin U.
- INFN, Rome2; Rome Observ.; INFN, Perugia
- Bologna Observ.; Bologna U.
- INFN, Trieste
- INFN, Bari; Naples U.
- INFN, Trieste; Udine U.
- Bari U.
- Fermilab
- SUNY, Stony Brook
- Bari U.; INFN, Bari
- Hiroshima U.
- Bologna Observ.
- INFN, Rome; Chile U., Catolica
- DAPNIA, Saclay
- Gottingen U.
- Maryland U., Baltimore County; NASA, Goddard
- Iceland U.
- INFN, Turin
- Barcelona, IEEC
- Royal Inst. Tech., Stockholm; Stockholm U., OKC
- NASA, Goddard; Maryland U.
- INFN, Rome
- UC, Irvine
- Denver U.
- Munich, Max Planck Inst.; Stanford U., HEPL; KIPAC, Menlo Park; Stanford U., Phys. Dept.
- Innsbruck U.; Stanford U., HEPL; KIPAC, Menlo Park; Stanford U., Phys. Dept.
- Stockholm U., OKC; Stockholm U.
- Friends Academy, Locust Valley
- Texas A-M
- Nagoya U., Solar-Terrestrial Environ. Lab.; Stanford U., HEPL; KIPAC, Menlo Park; Stanford U., Phys. Dept.
- Barcelona, IEEC; ICREA, Barcelona
- Innsbruck U.
- Ohio State U., CCAPP
- Naval Research Lab, Wash., D.C.
- INFN, Trieste; Nova Gorica U.
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.
- Research Organization:
- Barcelona, IEEC; Bari U.; Bologna Observ.; Bologna U.; Brera Observ.; CIFS, Turin; Chicago U., KICP; Chile U., Catolica; DAPNIA, Saclay; DESY; Denver U.; Ecole Polytechnique; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Friends Academy, Locust Valley; George Washington U.; Gottingen U.; Hiroshima U.; ICREA, Barcelona; INFN, Bari; INFN, Padua; INFN, Perugia; INFN, Pisa; INFN, Rome; INFN, Rome2; INFN, Trieste; INFN, Turin; Iceland U.; Innsbruck U.; Maryland U.; Maryland U., Baltimore County; Munich, Max Planck Inst.; NASA, Goddard; Nagoya U., Solar-Terrestrial Environ. Lab.; Naples U.; Naval Research Lab, Wash., D.C.; Nova Gorica U.; Ohio State U., CCAPP; Padua U.; Perugia U.; Rome Observ.; Royal Inst. Tech., Stockholm; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); SUNY, Stony Brook; Stanford U., HEPL; Stanford U., Phys. Dept.; Stockholm U.; Stockholm U., OKC; Texas A-M; Trieste U.; Turin U.; U. Montpellier 2, LUPM; UC, Irvine; UC, Santa Cruz; Udine U.
- Sponsoring Organization:
- US Department of Energy; USDOE
- Contributing Organization:
- The Fermi-LAT Collaboration
- Grant/Contract Number:
- AC02-07CH11359; AC02-76SF00515
- OSTI ID:
- 1234886
- Alternate ID(s):
- OSTI ID: 1227524
OSTI ID: 1354855
- Report Number(s):
- FERMILAB-PUB-15-081-AE; oai:inspirehep.net:1351193; arXiv:1503.02641
- Journal Information:
- Phys.Rev.Lett., Journal Name: Phys.Rev.Lett. Journal Issue: 23 Vol. 115
- Country of Publication:
- United States
- Language:
- English
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