Pascale Jablonka
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Expertise Formation and evolution of galaxies: surveys and numerical simulations.Galaxy clusters and cosmic filamentary structuresLocal Group dwarf galaxiesFirst generations of stars in the Universe Expertise Formation and evolution of galaxies: surveys and numerical simulations.Galaxy clusters and cosmic filamentary structuresLocal Group dwarf galaxiesFirst generations of stars in the Universe Research Project If you are looking for aTPIV or Master project ; if you are interested in image processing, deep learning, spectroscopic, or photometric methods applied to galaxy transformations in the cosmic web, the formation and evolution of dwarf galaxies, or the nature of the first stars, don't hesitate to contact me. Pascale Jablonka is a French/Swiss astrophysicist who specializes in the area of galaxy evolution. She earned a doctorate in astrophysics from the University Paris 7- Denis Diderot in France. She then held a postdoctoral fellowship at the Headquarter of the European Southern Observatory (ESO, Germany), before obtaining a position at CNRS (France). She is currently Directrice de Recherche at CNRS and on leave of absence from Paris Observatory in the Laboratory of Astrophysics at EPFL. Teaching & PhD PhD Students Robert Daniel Kincaid, Markus Johan Bredberg Past EPFL PhD Students Damien Spérone-Longin, Romain Ely Roland Lucchesi, Nick Heesters, Utsav Akhaury Past EPFL PhD Students as codirector Martin Tafelmeyer, François Henri Ambroise Rérat, Romaine Theler Courses Astrophysics II : interactions radiation-matter PHYS-472 This course provides the essential concepts for understanding how stars form, evolve, radiate, and synthesize their chemical elements. These are fundamentals to tackle the variety of galaxy properties, and how their interstellar medium is gradually enriched with metals. History of cosmology UNIL-002 This course illustrates, in a simplified but nevertheless correct way, the results of the scientific method applied to the study of the Universe, from Greek Antiquity to recent progress in cosmology, fruits of the confrontation of theory and observation.
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