activity
20032009
most citedMeasurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope

911 citations · 1.9k across the 24 of their papers we have counts for

collaborators
Showing 2003Show all

5 papers · 1 filter

astro-ph20032 cited

Antiprotons in CR: What Do They Tell Us?

I. V. Moskalenko, A. W. Strong, S. G. Mashnik +1

Recent measurements of the CR antiproton flux have been shown to pose a problem for conventional propagation models. In particular, models consistent with secondary/primary nuclei…

astro-ph200316 cited

Evaluation of Production Cross Sections of Li, Be, B in CR

I. V. Moskalenko, S. G. Mashnik

Accurate evaluation of production cross sections of light elements is important for models of CR propagation, galactic chemical evolution, and cosmological studies. However, experi…

astro-ph20033 cited

Propagation of Light Elements in the Galaxy

I. V. Moskalenko, A. W. Strong, S. G. Mashnik +1

The origin and evolution of isotopes of the lightest elements H2, He3, Li, Be, B in the universe is a key problem in such fields as astrophysics of CR, Galactic evolution, non-ther…

astro-ph20032 cited

Evaluation of Models for Diffuse Continuum Gamma Rays in EGRET Range

A. W. Strong, I. V. Moskalenko, O. Reimer

The GALPROP model for cosmic-ray (CR) propagation produces explicit predictions for the angular distribution of Galactic diffuse gamma rays. We compare our current models with EGRE…

astro-ph20032 cited

A New Estimate of the Extragalactic Gamma-Ray Background from EGRET Data

A. W. Strong, I. V. Moskalenko, O. Reimer

We use the GALPROP model for cosmic-ray (CR) propagation to obtain our best prediction of the Galactic component of gamma rays, and show that away from the Galactic plane it gives…