Curso de Astropartículas y Rayos Cósmicos
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Updated
Apr 5, 2021
Curso de Astropartículas y Rayos Cósmicos
Predictive Uncertainty in Gradient-Boosted Regression Trees : A Muon Energy Reconstruction Case Study
Positron's Milky Way Energy Loss using Operator learning
The LAGO Project Astroparticle physics course
Simulation of the Optics of the Imaging Air-Cherenkov Telescopes IceAct with Geant4
Analysis pipeline capable of searching for dark compact objects in the Milky Way through astrometric lensing in real or mock Gaia DR4 data.
Simplified cosmic-ray measurement database
Astrophysical Neutrino Anisotropy
This library contains the p+p->gamma production cross sections implemented in Python, C/C++, Fortran and Matlab. For details, see Phys.Rev. D90 (2014) 12, 123014
Dark Matter Simulation Code for Underground Scatterings
This project is an astrophysical research that study a self-proposed semi-analytical method to simulate solar asmospheric gamma-ray flux.
Characterisation and detection of radiation at radio frequencies in cascades initiated by very high energies Cosmic Rays and Neutrinos
Code to compute the self-generated TeV halos around pulsars
Database of published cosmic-ray energy spectra
Simulation of the detector for the GRAMS experiment
SimProp is a Monte Carlo simulation code of ultra-high energy cosmic ray propagation.
Deconvolution algorithms popular in Cherenkov astronomy
A framework designed to simulate the signals produced by the secondary particles emerging from the interaction of the flux of primary cosmic ray with the atmosphere. These signals are simulated for any particle detector located at any place (latitude, longitude and altitude), including the real-time atmospheric, geomagnetic and detector conditions.
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