Global Spline Fit: A unified data-driven view of the cosmic-ray spectrum and mass composition from GeV to the highest energies
astro-ph.HE
Submitted: 2026-09-26
Updated: 2026-09-26
Terminology
Sources
- The origin of Galactic cosmic rays: challenges to the standard paradigm
- On the knee in the energy spectrum of cosmic rays
- Spectrum of cosmic-ray nucleons and the atmospheric muon charge ratio
- Cosmic Ray Energy Spectrum from Measurements of Air Showers
- Flux of Atmospheric Neutrinos
- Three component model of cosmic ray spectra from 10 GeV to 100 PeV
- Precise measurement of the cosmic-ray spectrum and $\left \langle \ln A \right \rangle$ by LHAASO -- connecting the Galactic to the extragalactic components
- The IceCube Neutrino Observatory: Instrumentation and Online Systems
- Letter of Intent for KM3NeT 2.0
- Neutrino Telescope in Lake Baikal: Present and Nearest Future
- The Pacific Ocean Neutrino Experiment
- A multi-cubic-kilometre neutrino telescope in the western Pacific Ocean
- The Muon Puzzle in cosmic-ray induced air showers and its connection to the Large Hadron Collider
- Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeV
- Towards the Composition of sub-PeV Cosmic Rays at IceCube
- Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track Samples
- Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV
- News from Cosmic Ray Air Showers (ICRC 2019 -- Cosmic Ray Indirect Rapport)
- Precision spectral measurements of Chromium and Titanium from 10 to 250 GeV$/n$ and sub-Iron to Iron ratio with the Calorimetric Electron Telescope on the ISS
- Neutron monitors and muon detectors for solar modulation studies: 2. $\phi$ time series
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