KiDS-1000 cosmology: Cosmic shear constraints and comparison between two point statistics
Royal Observatory · University of Edinburgh · +14 more institutions
Abstract
We present cosmological constraints from a cosmic shear analysis of the fourth data release of the Kilo-Degree Survey (KiDS-1000), which doubles the survey area with nine-band optical and near-infrared photometry with respect to previous KiDS analyses. Adopting a spatially flat standard cosmological model, we find S 8 = σ 8 (Ω m /0.3) 0.5 = 0.759 −0.021 +0.024 for our fiducial analysis, which is in 3 σ tension with the prediction of the Planck Legacy analysis of the cosmic microwave background. We compare our fiducial COSEBIs (Complete Orthogonal Sets of E/B-Integrals) analysis with complementary analyses of the two-point shear correlation function and band power spectra, finding the results to be in excellent…
Citation impact
- FWCI
- 47.90
- Percentile
- 100%
- References
- 161
Authors
25- MAMarika AsgariCorresponding
Royal Observatory, University of Edinburgh
- CLChieh-An Lin
Royal Observatory, University of Edinburgh
- BJBenjamin Joachimi
University College London
- BGBenjamin Giblin
Royal Observatory, University of Edinburgh
- CHCatherine Heymans
Royal Observatory, Ruhr University Bochum, University of Edinburgh
Topics & keywords
- Physics
- Astrophysics
- Cosmic microwave background
- COSMIC cancer database
- Planck
- Cosmology
- Omega
- Spectral density
- Reduced inequalities
Funding
- AVAlexander von Humboldt-Stiftung
- ECEuropean CommissionAwards: 647112, 797794, 770935
- DFDeutsche ForschungsgemeinschaftAwards: 770935, 1495/5-1, Hi 1495/5-1, 639.043.512
- NNNational Natural Science Foundation of ChinaAwards: 11973070, 19ZR1466600, ZDBS-LY-7013
- BFBundesministerium für Bildung und Forschung
- NONederlandse Organisatie voor Wetenschappelijk OnderzoekAwards: 639.043.512, 621.016.402, Vici grant 639.043.512
- MMax-Planck-Gesellschaft
- SAScience and Technology Facilities CouncilAwards: ST/N000919/1, DIR/WK/2018/12, ST/N000919/1, 2018/31/G/ST9/03388, ST/S000488/1
- IAINAF-Osservatorio Astronomico di Padova
- NNNational Natural Science Foundation of China-Guangdong Joint FundAward: 11973070
- HMH2020 Marie Skłodowska-Curie ActionsAward: 797794