UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

Abbott, TMC; Abdalla, FB; Alarcon, A; Allam, S; Annis, J; Avila, S; Aylor, K; ... Zuntz, J; + view all (2019) Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions. Physical Review D , 100 (2) , Article 023541. 10.1103/PhysRevD.100.023541. Green open access

[thumbnail of Abdalla_Dark Energy Survey year 1 results. Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions_VoR.pdf]
Preview
Text
Abdalla_Dark Energy Survey year 1 results. Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions_VoR.pdf - Published Version

Download (1MB) | Preview

Abstract

We perform a joint analysis of the auto and cross-correlations between three cosmic fields: the galaxy density field, the galaxy weak lensing shear field, and the cosmic microwave background (CMB) weak lensing convergence field. These three fields are measured using roughly 1300 sq. deg. of overlapping optical imaging data from first year observations of the Dark Energy Survey (DES) and millimeter-wave observations of the CMB from both the South Pole Telescope Sunyaev-Zel’dovich survey and Planck. We present cosmological constraints from the joint analysis of the two-point correlation functions between galaxy density and galaxy shear with CMB lensing. We test for consistency between these measurements and the DES-only two-point function measurements, finding no evidence for inconsistency in the context of flat Λ CDM cosmological models. Performing a joint analysis of five of the possible correlation functions between these fields (excluding only the CMB lensing autospectrum) yields S₈ ≡ σ₈ √Ω_{m}/0.3 = 0.782 ⁺⁰·⁰¹⁹_₀.₀₂₅ and Ω_{m} = 0.260 ⁺⁰·⁰²⁹_₀.₀₁₉. We test for consistency between these five correlation function measurements and the Planck-only measurement of the CMB lensing autospectrum, again finding no evidence for inconsistency in the context of flat Λ CDM models. Combining constraints from all six two-point functions yields S₈ = 0.776 ⁺⁰·⁰¹⁴_₀.₀₂₁ and Ω = 0.271 ⁺⁰·⁰²²_₀.₀₁₆. These results provide a powerful test and confirmation of the results from the first year DES joint-probes analysis.

Type: Article
Title: Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions
Open access status: An open access version is available from UCL Discovery
DOI: 10.1103/PhysRevD.100.023541
Publisher version: https://doi.org/10.1103/PhysRevD.100.023541
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.
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/10079500
Downloads since deposit
49Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item