HCERES meeting at LAM
Laboratory visit by the HCERES committee: presentations, visits, meetings as announced by email.
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PhD Defense by Lorena Acuna
PhD Defense by Lorena Acuna
"Modelling the populations of low-mass planets: transition between super-Earths and mini-Neptunes" Zoom link: https://univ-amu-fr.zoom.us/j/88020777410?pwd=WlNQL1VyYWxOQjFaQ1pnU0I3SUpPdz09 Abstract Low-mass exoplanets are showing a diversity in their densities and irradiation conditions, ranging from highly irradiated planets to temperate worlds. To estimate their composition, we have developed an interior structure model that includes self-consistently an atmosphere in radiative-convective equilibrium. The […]
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PhD defense by Artem Aguichine
PhD defense by Artem Aguichine
"Retracing the fate of volatile compounds: from circumstellar disks to planetary interiors" zoom: https://univ-amu-fr.zoom.us/j/89671630809?pwd=Q2Jhbkd5cWZHU3VuS3lyVUVrWGhyQT09 Abstract: Volatile compounds are a part of the elementary blocks in planet formation, and are also essentials for the formation of life. Understanding how they are redistributed in protostellar disks gives valuable information on planet formation mechanisms, which can then be […]
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PhD defense: Gayathri Gururajan
PhD defense: Gayathri Gururajan
"Probing the gas reservoirs of high redshift, dusty star-forming galaxies using ALMA observations of atomic carbon" Here is the zoom link for those who are willing to attend remotely : https://univ-amu-fr.zoom.us/j/7585591256 Abstract: Intensely star-forming (> 500 M⦿/yr) dusty galaxies are found in the early Universe, and many questions regarding their formation and mass assembly remain […]
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Thesis defense by Neda Heidari
Thesis defense by Neda Heidari
"Overcoming the stellar activity impact on exoplanet detection and characterization". The defense will be held in English. Please find below the Ph.D. thesis abstract and the jury members. Lien zoom: https://univ-amu-fr.zoom.us/j/84199793791?pwd=VjhXbkpFditIM0dUWitRaFFkL1YyZz09 Abstract: Low-mass planets, with a mass of lower than 30 Earth masses, have an extraordinarily diverse range in terms of compositions. Their bulk density, […]
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