Présidents de session
The Galaxy Clustering Spec (GCsp) probe, reference model and performances
- Martin Crocce
Description
Presentation of the GC spectroscopic reference model its performances in terms of FoM, dependence on priors, etc.
Dr
Santiago Casas
(TTK, RWTH Aachen University)
21/03/2023 09:00
CLOE, status and performances
We expand and adjust the synthetic Euclid likelihoods of the MontePython software in order to match the exact recipes used
in previous Euclid Fisher matrix forecasts for several probes: weak lensing cosmic shear, photometric galaxy clustering, the cross-
correlation between the latter observables, and spectroscopic galaxy clustering. We also establish which precision settings are
required...
