Orateur
Michel-Andrès Breton
(Laboratoire d'Astrophysique de Marseille)
Description
In this talk I will discuss about the impact of magnification bias on the determination of the growth rate from redshift-space clustering. We use a the RayGal suite of $N$-body simulations that accounts for the fully non-linear structure formation and perform realistic galaxy clustering analyses, similarly as in observations, in different regime of magnification bias. We investigate a minimal model to account for the magnification effect on the multipole moments of the redshift-space correlation function, and study the accuracy with which the the growth rate of structure parameter can be recovered.
Auteur principal
Michel-Andrès Breton
(Laboratoire d'Astrophysique de Marseille)
Co-auteurs
Sylvain de la Torre
(LAM)
Jade Piat
(LAM)