pith. machine review for the scientific record. sign in

arxiv: 1008.3642 · v3 · submitted 2010-08-21 · 🌌 astro-ph.HE · astro-ph.GA· physics.comp-ph

Recognition: unknown

GALPROP WebRun: an internet-based service for calculating galactic cosmic ray propagation and associated photon emissions

Authors on Pith no claims yet
classification 🌌 astro-ph.HE astro-ph.GAphysics.comp-ph
keywords galpropcodepropagationserviceavailablecalculatingcosmicemissions
0
0 comments X
read the original abstract

GALPROP is a numerical code for calculating the galactic propagation of relativistic charged particles and the diffuse emissions produced during their propagation. The code incorporates as much realistic astrophysical input as possible together with latest theoretical developments and has become a de facto standard in astrophysics of cosmic rays. We present GALPROP WebRun, a service to the scientific community enabling easy use of the freely available GALPROP code via web browsers. In addition, we introduce the latest GALPROP version 54, available through this service.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons

    astro-ph.HE 2026-04 unverdicted novelty 5.0

    The bow shock pulsar wind nebula around PSR J0437-4715 explains the GeV-TeV positron excess and hundreds-of-GeV antiproton flux with an energy-independent ratio by using 25% of the pulsar's wind power.