Add to ORKGAbstract: StellarICs is software to compute gamma-ray emission from inverse-Compton scattering by cosmic-ray leptons in the heliosphere and in the photospheres of stars. It includes a set of cosmic-ray spectra and a formulation of their modulation, but it can be used for any user-defined modulation model and lepton spectra. Inverse-Compton emission provides a unique probe of cosmic-ray leptons in the heliosphere between the earth and the sun. The software is publicly available and it is under continuing development
Abstract: The Cygnus region is an extremely active star forming region with a wealth of gamma-ray so...
Abstract: The design of the new space-based gamma-ray telescope GAMMA-400 is presented. GAMMA-400 is...
Abstract: With its high-precision measurement of the cosmic-ray antiproton spectrum and sensitive se...
Abstract: StellarICs is software to compute gamma-ray emission from inverse-Compton scattering by co...
We present our software to compute gamma-ray emission from inverse-Compton scattering by cosmic-ray ...
Abstract: More than 90 % of the Galactic gas-related γ-ray emissivity above 1 GeV is attributed to t...
Abstract: The GALPROP project celebrates its 17th anniversary this year. It is devoted to the develo...
Using diffuse radio emission in clusters of galaxies to probe the cosmic web, cosmic rays and dark m...
Abstract: GAMMA-400 is a future high-energy γ-ray telescope, designed to measure the fluxes of γ-ray...
Abstract: Diffuse γ-ray emission has long been established as the most prominent feature in the GeV ...
Abstract: The last decade has been dense with new developments in the search for the sources of Gala...
Abstract: JEM-EUSO is a space telescope to be installed at the International Space Station to observ...
Abstract: Thanks to the success of current gamma-ray telescopes (Fermi, H.E.S.S., MAGIC, VERITAS), a...
Abstract: Very high energy (VHE) diffuse gamma-ray emission measurements are an excellent probe of c...
9The Sun is a known quiescent gamma-ray source. Its gamma-ray steady-state, characterized by two dis...
Abstract: The Cygnus region is an extremely active star forming region with a wealth of gamma-ray so...
Abstract: The design of the new space-based gamma-ray telescope GAMMA-400 is presented. GAMMA-400 is...
Abstract: With its high-precision measurement of the cosmic-ray antiproton spectrum and sensitive se...
Abstract: StellarICs is software to compute gamma-ray emission from inverse-Compton scattering by co...
We present our software to compute gamma-ray emission from inverse-Compton scattering by cosmic-ray ...
Abstract: More than 90 % of the Galactic gas-related γ-ray emissivity above 1 GeV is attributed to t...
Abstract: The GALPROP project celebrates its 17th anniversary this year. It is devoted to the develo...
Using diffuse radio emission in clusters of galaxies to probe the cosmic web, cosmic rays and dark m...
Abstract: GAMMA-400 is a future high-energy γ-ray telescope, designed to measure the fluxes of γ-ray...
Abstract: Diffuse γ-ray emission has long been established as the most prominent feature in the GeV ...
Abstract: The last decade has been dense with new developments in the search for the sources of Gala...
Abstract: JEM-EUSO is a space telescope to be installed at the International Space Station to observ...
Abstract: Thanks to the success of current gamma-ray telescopes (Fermi, H.E.S.S., MAGIC, VERITAS), a...
Abstract: Very high energy (VHE) diffuse gamma-ray emission measurements are an excellent probe of c...
9The Sun is a known quiescent gamma-ray source. Its gamma-ray steady-state, characterized by two dis...
Abstract: The Cygnus region is an extremely active star forming region with a wealth of gamma-ray so...
Abstract: The design of the new space-based gamma-ray telescope GAMMA-400 is presented. GAMMA-400 is...
Abstract: With its high-precision measurement of the cosmic-ray antiproton spectrum and sensitive se...