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The past decade has brought impressive advances in the astrophysics of cosmicrays (CRs) and multiwavelength astronomy, thanks to the new instrumentationlaunched into space and built on the ground. Modern technologies employed bythose instruments provide measurements with unmatched precision, enablingsearches for subtle signatures of dark matter (DM) and new physics.Understanding the astrophysical backgrounds to better precision than theobserved data is vital in moving to this new territory. The state-of-the-art CRpropagation code called GALPROP is designed to address exactly this challenge.Having 25 years of development behind it, the GALPROP framework has become ade-facto standard in the astrophysics of CRs, diffuse photon emissions (radio-to gamma-rays), and searches for new physics. GALPROP uses information fromastronomy, particle physics, and nuclear physics to predict CRs and theirassociated emissions self-consistently, providing a unifying modellingframework. The range of its physical validity covers 18 orders of magnitude inenergy, from sub-keV to PeV energies for particles and from micro-eV to PeVenergies for photons. The framework and the datasets are public and areextensively used by many experimental collaborations and by thousands ofindividual researchers worldwide for interpretation of their data and formaking predictions. This paper details the latest release of the GALPROPframework and updated cross sections, further developments of its initiallyauxiliary datasets for models of the interstellar medium that grew intoindependent studies of the Galactic structure -- distributions of gas, dust,radiation and magnetic fields -- as well as the extension of its modellingcapabilities. Example applications included with the distribution illustratingusage of the new features are also described.

The GALPROP Cosmic-ray Propagation and Non-thermal Emissions Framework: Release v57