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The effects of varying depth in cosmic shear surveys

Heydenreich, S; Schneider, P; Hildebrandt, H; Asgari, M; Heymans, C; Joachimi, B; Kuijken, K; ... Van den Busch, JL; + view all (2019) The effects of varying depth in cosmic shear surveys. Astronomy & Astrophysics 10.1051/0004-6361/201936966. (In press). Green open access

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Abstract

We present a semi-analytic model for the shear two-point correlation function of a cosmic shear survey with non-uniform depth. Ground-based surveys are subject to depth variations that primarily arise through varying atmospheric conditions. For a survey like the Kilo-Degree Survey (KiDS), we find that the measured depth variation increases the amplitude of the observed shear correlation function at the level of a few percent out to degree-scales, relative to the assumed uniform-depth case. The impact on the inferred cosmological parameters is shown to be insignificant for a KiDS-like survey. For next-generation cosmic shear experiments, however, we conclude that variable depth should be accounted for.

Type: Article
Title: The effects of varying depth in cosmic shear surveys
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/201936966
Publisher version: https://doi.org/10.1051/0004-6361/201936966
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: gravitational lensing: weak – cosmology: miscellaneous
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 Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10089010
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