Spectroscopy CFD Accretion Apprentissage profond Ab initio calculations Ab initio Density Functional Theory Modeling Nanoparticles Galaxies active Numerical simulations Instabilities Density functional calculations Deep Learning Numerical modelling Ligands Direct numerical simulation Deep learning Machine learning Protoplanetary disks Molecular dynamics simulations Modelling Hydrodynamics Large eddy simulation Climate change Mass spectrometry Machine Learning Channel flow Magnetohydrodynamics MHD Libre accès Calcul parallèle Dynamo Density functional theory Science ouverte Données de la recherche Supernovae general Hydrogen Adsorption Diffusion Aeroacoustics Catalysis HPC Simulation numérique High performance computing Stars formation Accretion disks France Galaxies evolution Combustion Open science Methods numerical Astrochemistry Optimization Numerical modeling Computational seismology Wave propagation Numerical simulation Modélisation numérique 3D Galaxies high-redshift Atomization Parallel computing Heat transfer Open access Direct Numerical Simulation LES DNS Galaxies formation MPI Dynamo theories and simulations Molecular Dynamics Convection Simulation Dynamique moléculaire Astrophysics - Astrophysics of Galaxies DFT calculations RANS Radiative transfer Large-Eddy Simulation Modélisation Electronic structure Iron Luminescence COVID-19 Inverse theory Calcul haute performance Quantum chemistry DFT Two-phase flow Copper Molecular dynamics Cosmology theory MHD Magnetic fields Data assimilation Palladium Large-scale structure of Universe Large Eddy Simulation Large-eddy simulation Turbulence