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20032019
most citedMeasurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

911 citations · 1.4k across the 7 of their papers we have counts for

collaborators

7 papers

physics.ins-det2019★ 37 cited

Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units

KM3NeT Collaboration, M. Ageron, S. Aiello +262

KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collabora…

astro-ph.HE2017★ 53 cited

New Constraints on all flavour Galactic diffuse neutrino emission with the ANTARES telescope

A. Albert, M. André, M. Anghinolfi +126

The flux of very high-energy neutrinos produced in our Galaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. The characterization…

astro-ph.HE2015

Gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV

Daniele Gaggero, Dario Grasso, Antonio Marinelli +2

As recently shown, Fermi-LAT measurements of the diffuse gamma-ray emission from the Galaxy favor the presence of a smooth softening in the primary cosmic-ray spectrum with increas…

astro-ph.HE2012★ 29 cited

Detection Potential of the KM3NeT Detector for High-Energy Neutrinos from the Fermi Bubbles

The KM3NeT Collaboration

A recent analysis of the Fermi Large Area Telescope data provided evidence for a high-intensity emission of high-energy gamma rays with a E^-2 spectrum from two large areas, spanni…

astro-ph.HE2009★ 911 cited

Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

LAT Collaboration

Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2m^2 sr at 300 GeV. Building on…

astro-ph2004★ 335 cited

Constrained Simulations of the Magnetic Field in the Local Universe and the Propagation of UHECRs

Klaus Dolag, Dario Grasso, Volker Springel +1

We use simulations of LSS formation to study the build-up of magnetic fields (MFs) in the ICM. Our basic assumption is that cosmological MFs grow in a MHD amplification process dri…