The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark Matter Annihilation
M. Ajello(Azienda Ospedaliera Citta' della Salute e della Scienza di Torino), Roger W. Romani(Kavli Institute for Particle Astrophysics and Cosmology), D. Gasparrini(Agenzia Spaziale Italiana), K. Bechtol(University of Wisconsin System), M. Ackermann(Deutsches Elektronen-Synchrotron DESY), A. W. Strong(Max Planck Institute for Extraterrestrial Physics), A. Franckowiak(SLAC National Accelerator Laboratory), D. H. Hartmann(Clemson University), C. D. Dermer(United States Naval Research Laboratory), A. Reimer(SLAC National Accelerator Laboratory), G. Zaharijaš(University of Nova Gorica), J. Cohen-Tanugi(Centre National de la Recherche Scientifique), M. Sánchez‐Conde(Stockholm University), M. Gustafsson(Université Libre de Bruxelles)
DESY Publication Database (PUBDB) (Deutsches Elektronen-Synchrotron)
February 20, 2015
Cited by 192
Related Papers
How Massive Single Stars End Their Life
|The Astrophysical Journal|2003|2.2k
Cosmic-Ray Propagation and Interactions in the Galaxy
|Annual Review of Nuclear and Particle Science|2007|1.1k
Propagation of Cosmic‐Ray Nucleons in the Galaxy
|The Astrophysical Journal|1998|1.1k
THE SPECTRUM OF ISOTROPIC DIFFUSE GAMMA-RAY EMISSION BETWEEN 100 MeV AND 820 GeV
|The Astrophysical Journal|2015|812
Radioactive 26Al from massive stars in the Galaxy
|Nature|2006|773