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Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear

Shaikh, S; Harrison, I; Van Engelen, A; Marques, GA; Abbott, TMC; Aguena, M; Alves, O; ... Smith, M; + view all (2024) Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear. Monthly Notices of the Royal Astronomical Society , 528 (2) pp. 2112-2135. 10.1093/mnras/stad3987. Green open access

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Abstract

Cross-correlation between weak lensing of the Cosmic Microwave Background (CMB) and weak lensing of galaxies offers a way to place robust constraints on cosmological and astrophysical parameters with reduced sensitivity to certain systematic effects affecting individual surveys. We measure the angular cross-power spectrum between the Atacama Cosmology Telescope (ACT) DR4 CMB lensing and the galaxy weak lensing measured by the Dark Energy Survey (DES) Y3 data. Our baseline analysis uses the CMB convergence map derived from ACT-DR4 and Planck data, where most of the contamination due to the thermal Sunyaev Zel’dovich effect is removed, thus avoiding important systematics in the cross-correlation. In our modelling, we consider the nuisance parameters of the photometric uncertainty, multiplicative shear bias and intrinsic alignment of galaxies. The resulting cross-power spectrum has a signal-to-noise ratio = 7.1 and passes a set of null tests. We use it to infer the amplitude of the fluctuations in the matter distribution (S8 ≡ σ8(Ωm/0.3)0.5 = 0.782 ± 0.059) with informative but well-motivated priors on the nuisance parameters. We also investigate the validity of these priors by significantly relaxing them and checking the consistency of the resulting posteriors, finding them consistent, albeit only with relatively weak constraints. This cross-correlation measurement will improve significantly with the new ACT-DR6 lensing map and form a key component of the joint 6×2pt analysis between DES and ACT.

Type: Article
Title: Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stad3987
Publisher version: https://doi.org/10.1093/mnras/stad3987
Language: English
Additional information: Copyright © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: Gravitational lensing: weak, large-scale structure of Universe, cosmology: observations, cosmological parameters
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.ucl.ac.uk/id/eprint/10187500
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