Explore projects

The aim of this project is to provide an illustrative demo on how to construct an observationally-driven population of Galactic (detached) double white dwarfs based on results derived from electromagnetic observations.

Présentation de janvier 2023 au sein du LPC, pour l'équipe INDRA-FAZIA. Dans celle-ci, je présente les avancements de ma thèse par rapport à mon stage.

The main idea behind the conception of this ETC (Exposure Time Calculator) is to provide a fast tool to estimate the NISP performances. This project is a fork of the Benoit Serra's code: https://marren.in2p3.fr/svn/Euclid/NISP/sw/etc/

Detection of cyclone using IASI data and Yolo model.

Tutorial on the Urban Heat Island (UHI) effect based on an application to the Paris area using Land Surface Temperature (LST) from satellite data.

Multi Chain Monte Carlo Markov Chain

Framework to derive constraints on the (velocity-independent) dark matter pair-annihilation cross-section utilising Fermi-LAT gamma-ray data of Milky Way dwarf spheroidal galaxies based on machine learning-optimized background assessment

https://tutoriels-jupyter.pages.in2p3.fr/2022-12-14-OSD-UGA