Line shape parameters Stars interiors Soutenance2022 Methane Low temperatures Low temperature chemistry Molecular processes Laboratory astrophysics Astrophysics Collisional Catalogs Shock waves Reaction kinetics Astrophysics - Solar and Stellar Astrophysics Fourier transform infrared spectroscopy Molecular data Feshbach resonances Collisional cross sections Cold and ultra-cold collisions Soutenance2021 Molecular collisions Spectral line shape Spectroscopy Pressure broadening Ozonolysis Binaries spectroscopic Hydrogen Astrochemistry Ab initio calculations Molecular physics ISM clouds Nanoparticles Astrophysics - Astrophysics of Galaxies Probes Methods numerical Artificial Neuron Networks ANN Contact resistance PhDtitle Optical-optical double resonance spectroscopy Branching ratio Rate coefficients Stars oscillations SAXS ISM molecules MCTDH Scattering Stars formation Kinetics Methods analytical ISM abundances Combustion Collisional broadening Reaction products Microwave spectroscopy Contact voltage Reaction kinetics and dynamics Vibronic couplings Stars solar-type Planetary atmospheres Optical frequency comb spectroscopy Line profiles Stars evolution Computational chemistry Methods data analysis Stars fundamental parameters Reaction dynamics Helium clusters CRESU Potential energy surfaces Radiative transfer Radio lines ISM Line-shape parameters Radial velocities Fretting corrosion Spectral element methods Plasma plume Proper motions Cold collisions Atomic and molecular collisions Potential energy Astrophysics laboratory Chemical physics Quantum theory Nitrogen Quantum chemistry Molecular data -molecular processes -ISM Molecules He Low temperature chemical kinetics Surveys Spectrometers Quantum dynamics Atomic and molecular physics Collisions Asteroseismology Titan Quantum Monte Carlo Chemical kinetics Astrometry Linewidths