Euclid preparation. VI. Verifying the performance of cosmic shear experiments
Aims: Our aim is to quantify the impact of systematic effects on the inference of cosmological parameters from cosmic shear. Methods: We present an "end-to-end" approach that introduces sources of bias in a modelled weak lensing survey on a galaxy-by-galaxy level. We propagated residual biases through a pipeline from galaxy properties at one end to
Euclid Collaboration et al.
Fecha de publicación:
3
2020