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.
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Dr Santiago Casas (TTK, RWTH Aachen University)21/03/2023 09:00CLOE, status and performances
We expand and adjust the synthetic Euclid likelihoods of the MontePython software in order to match the exact recipes used
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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...