Rubin LSST-France, CC-IN2P3 Lyon, 13-15/12/2023

ZTF instrument model

Non programmé

20m

Amphithéâtre (Centre de Calcul de l'IN2P3)

Parallel work sessions

Orateur

Philippe Rosnet (Laboratoire de Physique de Clermont, Université Clermont Auvergne & CNRS/IN2P3)

Description

The ZTF-IN2P3 effort to achieve a photometric precision at the permile level for cosmology studies with type Ia supernova leads to the development of a model of the instrument. This model is used to extrapolate the measured filter transmission performed at normal incident angle by Caltech to the typical incident angle of the P48 Schmidt telescope used by ZTF.