Zlata Kormilicina
Riga State Classical Gymnasium, Latvia
Abstract
Analysing type Ia Supernovas data we can compare it with different cosmological models, one of them being the ΛCDM model. Using a standard likelihood analyses, we explored a number of different ΛCDM models and its extensions to understand the constraining power of this data.
2026 July 24, 13:30
IA/U.Porto
Centro de Astrofísica da Universidade do Porto (Classroom)
Rua das Estrelas, 4150-762 Porto





