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Euclid preparation: VI. Verifying the performance of cosmic shear experiments

Paykari, P; Kitching, T; Hoekstra, H; Azzollini, R; Cardone, VF; Cropper, M; Duncan, CAJ; ... Zucca, E; + view all (2020) Euclid preparation: VI. Verifying the performance of cosmic shear experiments. Astronomy & Astrophysics , 635 , Article A139. 10.1051/0004-6361/201936980. Green open access

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Abstract

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 cosmic shear power spectra and cosmological parameter estimates at the other end. We did this to quantify how imperfect knowledge of the pipeline changes the maximum likelihood values of dark energy parameters. RESULTS: We quantify the impact of an imperfect correction for charge transfer inefficiency and modelling uncertainties of the point spread function for Euclid, and find that the biases introduced can be corrected to acceptable levels.

Type: Article
Title: Euclid preparation: VI. Verifying the performance of cosmic shear experiments
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/201936980
Publisher version: https://doi.org/10.1051/0004-6361/201936980
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher's terms and conditions.
Keywords: gravitational lensing: weak
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10094742
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