Search for Galactic PeV gamma rays with the IceCube Neutrino Observatory

5 Note added: While this work was being finalized for submission, an in-depth study of this effect has appeared as pre-print [25]... It has even been proposed that “GC shells”

matter annihilation cross section hσ A υi obtained for the combined analysis as a function of the dark matter mass m DM assuming the NFW halo profile for the τ þ τ −

The P toolset greatly benefits from the experience obtained during the GeneAuto project [1]. It is fair to say that the contents of this section are an evolution of those

We analyse the intensity of nuclear de-excitation lines in the direction of the Galactic center produced by subrelativistic protons, which are generated by star capture by the

Nous avons utilisé le logiciel SYMBOLS-2000 pour la simulation du circuit électrique équivalent de ce capteur SYMBOLS-2000 est un logiciel de simulation pour la modélisation Bond

1) Désignation et prix unitaire de tous les produits. 4) Nom des clients qui ont commandé au moins un produit de prix supérieur à 500 F. 5) Nom des clients qui n’ont pas

We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to

Considering that the level of di ff use Galactic emission in the TeV band approaches the level of residual cosmic-ray back- ground, we estimated the level of residual