Journal article
Euclid preparation: VI. Verifying the performance of cosmic shear experiments
- Abstract:
- Our aim is to quantify the impact of systematic effects on the inference of cosmological parameters from cosmic shear. We present an end-to-end approach that introduces sources of bias in a modelled weak lensing survey on a galaxy-by-galaxy level. Residual biases are propagated through a pipeline from galaxy properties (one end) through to cosmic shear power spectra and cosmological parameter estimates (the other end), to quantify how imperfect knowledge of the pipeline changes the maximum likelihood values of dark energy parameters. We quantify the impact of an imperfect correction for charge transfer inefficiency (CTI) and modelling uncertainties of the point spread function (PSF) for Euclid, and find that the biases introduced can be corrected to acceptable levels.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Version of record, pdf, 1.4MB, Terms of use)
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- Publisher copy:
- 10.1051/0004-6361/201936980
Authors
- Publisher:
- EDP Sciences
- Journal:
- Astronomy and Astrophysics More from this journal
- Volume:
- 635
- Issue:
- March 2020
- Pages:
- A139
- Publication date:
- 2020-03-23
- Acceptance date:
- 2020-01-26
- DOI:
- EISSN:
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1432-0746
- ISSN:
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0004-6361
- Language:
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English
- Keywords:
- Pubs id:
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1068199
- Local pid:
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pubs:1068199
- Deposit date:
-
2020-03-31
Terms of use
- Copyright holder:
- ESO
- Copyright date:
- 2020
- Rights statement:
- © ESO 2020
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