Pourvu:
Non
The abundance of galaxy clusters is a powerful probe for cosmology, especially on large-scale surveys. The goal will be to evaluate the impact of the different mass functions used for the theoretical prediction of cluster counts on the cosmological constraints. This project will be done for the preparation of the LSST-DESC cluster cosmology framework.
Responsable:
Simona Mei, Michel Aguena
Services/Groupes:
Année:
2023
Formations:
Stage