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

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.

Accepted for publication in Computer Physics Communications. Version 2 includes improvements suggested by the referee. Metadata completed in version 3 (no changes to the manuscript)

References in corpus (5)

• Global cosmic-ray related luminosity and energy budget of the Milky Way
• Inverse Compton Origin of the Hard X-Ray and Soft Gamma-Ray Emission from the Galactic Ridge
• Inverse Compton Emission from Galactic Supernova Remnants: Effect of the Interstellar Radiation Field
• Propagation of Light Elements in the Galaxy
• Isotopic composition of cosmic-ray sources

Cited by in corpus (148)

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• Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
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• A Global Analysis of Dark Matter Signals from 27 Dwarf Spheroidal Galaxies using 11 Years of Fermi-LAT Observations
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• Fermi-LAT Observations of Gamma-Ray Emission Towards the Outer Halo of M31
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• Possible Contribution to Electron and Positron Fluxes from Pulsars and their Nebulae
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• Galactic Gamma-Ray Diffuse Emission at TeV energies with HAWC Data
• Constraining the low-energy cosmic ray flux in the central molecular zone from MeV nuclear deexcitation line observations
• Cosmic rays: interstellar gamma-ray and radio emission
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• The Galactic Isotropic $\gamma$-ray Background and Implications for Dark Matter
• Improved Modeling of the Discrete Component of the Galactic Interstellar Gamma-ray Emission and Implications for the Fermi-LAT Galactic Center Excess
• Sources and Radiations of the Fermi Bubbles
• A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone
• Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data
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• Fermi Bubbles with HAWC
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• The low cosmic-ray density in Polaris Flare
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