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Search for gamma-ray emission from des dwarf spheroidal galaxy candidates with Fermi-LAT data

  • A. Drlica-Wagner
  • , A. Albert
  • , K. Bechtol
  • , M. Wood
  • , L. Strigari
  • , M. Sánchez-Conde
  • , L. Baldini
  • , R. Essig
  • , J. Cohen-Tanugi
  • , B. Anderson
  • , R. Bellazzini
  • , E. D. Bloom
  • , R. Caputo
  • , C. Cecchi
  • , E. Charles
  • , J. Chiang
  • , A. De Angelis
  • , S. Funk
  • , P. Fusco
  • , F. Gargano
  • N. Giglietto, F. Giordano, S. Guiriec, M. Gustafsson, M. Kuss, F. Loparco, P. Lubrano, N. Mirabal, T. Mizuno, A. Morselli, T. Ohsugi, E. Orlando, M. Persic, S. Rainò, N. Sehgal, F. Spada, D. J. Suson, G. Zaharijas, S. Zimmer, T. Abbott, S. Allam, E. Balbinot, A. H. Bauer, A. Benoit-Lévy, R. A. Bernstein, G. M. Bernstein, E. Bertin, D. Brooks, E. Buckley-Geer, D. L. Burke, A. Carnero Rosell, F. J. Castander, R. Covarrubias, C. B. D'Andrea, L. N.Da Costa, D. L. Depoy, S. Desai, H. T. Diehl, C. E. Cunha, T. F. Eifler, J. Estrada, A. E. Evrard, A. Fausti Neto, E. Fernandez, D. A. Finley, B. Flaugher, J. Frieman, E. Gaztanaga, D. Gerdes, D. Gruen, R. A. Gruendl, G. Gutierrez, K. Honscheid, B. Jain, D. James, T. Jeltema, S. Kent, R. Kron, K. Kuehn, N. Kuropatkin, O. Lahav, T. S. Li, E. Luque, M. A.G. Maia, M. Makler, M. March, J. Marshall, P. Martini, K. W. Merritt, C. Miller, R. Miquel, J. Mohr, E. Neilsen, B. Nord, R. Ogando, J. Peoples, D. Petravick, A. Pieres, A. A. Plazas, A. Queiroz, A. K. Romer, A. Roodman, E. S. Rykoff, M. Sako, E. Sanchez, B. Santiago, V. Scarpine, M. Schubnell, I. Sevilla, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E.C. Swanson, G. Tarle, J. Thaler, D. Thomas, D. Tucker, A. R. Walker, R. H. Wechsler, W. Wester, P. Williams, B. Yanny, J. Zuntz
  • Fermi National Accelerator Laboratory
  • Stanford University
  • The University of Chicago
  • Texas A&M University
  • Oskar Klein Centre
  • Stockholm University
  • University of Pisa
  • LUPM-UMR 5299, CNRS, Université Montpellier
  • National Institute for Nuclear Physics
  • University of California at Santa Cruz
  • University of Perugia
  • University of Udine
  • Polytechnic University of Bari
  • NASA Goddard Space Flight Center
  • University of Göttingen
  • Hiroshima University
  • Osservatorio Astronomico di Trieste
  • Purdue University Northwest
  • University of Trieste
  • University of Nova Gorica
  • National Optical Astronomy Observatory
  • Space Telescope Science Institute
  • University of Surrey
  • Laboratório Interinstitucional de e-Astronomia
  • CSIC
  • University College London
  • Carnegie Institution of Washington
  • University of Pennsylvania
  • Institut d'Astrophysique de Paris
  • SLAC National Accelerator Laboratory
  • Observatório Nacional
  • University of Illinois at Urbana-Champaign
  • University of Portsmouth
  • Excellence Cluster Universe
  • Ludwig Maximilian University of Munich
  • Jet Propulsion Laboratory, California Institute of Technology
  • University of Michigan, Ann Arbor
  • ICREA
  • Autonomous University of Barcelona
  • Max Planck Institute for Extraterrestrial Physics
  • Ohio State University
  • Australian Astronomical Observatory
  • Argonne National Laboratory
  • Universidade Federal do Rio Grande do Sul
  • Centro Brasileiro de Pesquisas Físicas
  • Brookhaven National Laboratory
  • University of Sussex
  • CIEMAT
  • University of Manchester

Research output: Contribution to journalArticlepeer-review

156 Scopus citations

Abstract

Due to their proximity, high dark-matter (DM) content, and apparent absence of non-thermal processes, Milky Way dwarf spheroidal satellite galaxies (dSphs) are excellent targets for the indirect detection of DM. Recently, eight new dSph candidates were discovered using the first year of data from the Dark Energy Survey (DES). We searched for gamma-ray emission coincident with the positions of these new objects in six years of Fermi Large Area Telescope data. We found no significant excesses of gamma-ray emission. Under the assumption that the DES candidates are dSphs with DM halo properties similar to the known dSphs, we computed individual and combined limits on the velocity-averaged DM annihilation cross section for these new targets. If the estimated DM content of these dSph candidates is confirmed, they will constrain the annihilation cross section to lie below the thermal relic cross section for DM particles with masses annihilating via the or τ+τ- channels.

Original languageEnglish
Article numberL4
JournalAstrophysical Journal Letters
Volume809
Issue number1
DOIs
StatePublished - Aug 10 2015

Keywords

  • Local Group
  • dark matter
  • galaxies: dwarf
  • gamma rays: galaxies

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