Add to ORKGAbstract: Interstellar synchrotron emission depends on Galactic magnetic fields and on cosmic-ray leptons. Observations of radio emission are an important tool for studying cosmic-ray propagation models and interstellar electron spectrum and distribution in the Galaxy. We present the latest developments in our modeling of Galactic synchrotron emission with the GALPROP code, including polarization, absorption, and free-free emission. Using surveys over a wide range of radio frequencies and polarization measurements, we derive constraints on the low-energy interstellar cosmic-ray electron spectrum, magnetic fields and cosmic-ray propagation models. This work is of interest for studies of interstellar gamma-ray emission with Fermi-LAT, and syn...
The interaction between the galactic magnetic field and the non-thermal population of electrons is r...
1Ever since the discovery of cosmic rays (CRs), significant advancements have been made in modelling...
Context.Our position inside the Galaxy requires 3D-modelling to obtain the distribution of the Gala...
Abstract: The GALPROP project celebrates its 17th anniversary this year. It is devoted to the develo...
Aims. We exploit synchrotron radiation to constrain the low-energy interstellar electron spectrum, u...
4Galactic cosmic rays (CR), interstellar gamma-ray emission and synchrotron radiation are related to...
1Galactic synchrotron radiation observed from radio to microwaves is produced by cosmic-ray (CR) ele...
8We use the GALPROP code for cosmic-ray (CR) propagation to calculate the broadband luminosity spect...
Abstract: We study the Galactic radio background produced by synchrotron emission of cosmic ray elec...
Abstract: More than 90 % of the Galactic gas-related γ-ray emissivity above 1 GeV is attributed to t...
The gamma-ray sky >100 MeV is dominated by the diffuse emissions from interactions of cosmic rays wi...
Context. Cosmic rays (CRs) and the Galactic magnetic field (GMF) are fundamental actors in many proc...
The interaction between the galactic magnetic field and the non-thermal population of electrons is r...
1Ever since the discovery of cosmic rays (CRs), significant advancements have been made in modelling...
Context.Our position inside the Galaxy requires 3D-modelling to obtain the distribution of the Gala...
Abstract: The GALPROP project celebrates its 17th anniversary this year. It is devoted to the develo...
Aims. We exploit synchrotron radiation to constrain the low-energy interstellar electron spectrum, u...
4Galactic cosmic rays (CR), interstellar gamma-ray emission and synchrotron radiation are related to...
1Galactic synchrotron radiation observed from radio to microwaves is produced by cosmic-ray (CR) ele...
8We use the GALPROP code for cosmic-ray (CR) propagation to calculate the broadband luminosity spect...
Abstract: We study the Galactic radio background produced by synchrotron emission of cosmic ray elec...
Abstract: More than 90 % of the Galactic gas-related γ-ray emissivity above 1 GeV is attributed to t...
The gamma-ray sky >100 MeV is dominated by the diffuse emissions from interactions of cosmic rays wi...
Context. Cosmic rays (CRs) and the Galactic magnetic field (GMF) are fundamental actors in many proc...
The interaction between the galactic magnetic field and the non-thermal population of electrons is r...
1Ever since the discovery of cosmic rays (CRs), significant advancements have been made in modelling...
Context.Our position inside the Galaxy requires 3D-modelling to obtain the distribution of the Gala...