An optimal quadratic estimator for window-free cosmic shear power spectra
Taisei Terawaki, Masahiro Takada
astro-ph.CO
Submitted: 2026-07-31
Comments: 13 pages, 8 figures
Code: https://github.com/LSSTDESC/NaMaster
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Weak lensing for precision cosmology
- Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions
- KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey
- Dark Energy Survey Year 6 Results: Cosmological Constraints from Cosmic Shear
- Analysis of two-point statistics of cosmic shear: I. Estimators and covariances
- Simulations of Wide-Field Weak Lensing Surveys II: Covariance Matrix of Real Space Correlation Functions
- Mock galaxy shape catalogs in the Subaru Hyper Suprime-Cam Survey
- B-modes in cosmic shear from source redshift clustering
- Power Spectra Estimation for Weak Lensing
- Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
- Power Spectrum Super-Sample Covariance
- Simulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian Effects
- The Impact of Non-Gaussian Errors on Weak Lensing Surveys
- CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys
- Weak Lensing On the Celestial Sphere
- Discriminating weak lensing from intrinsic spin correlations using the curl-gradient decomposition
- Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
- Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present
- A pseudo-spectrum analysis of galaxy-galaxy lensing
- The Pseudo-$C_l$ method: Cosmic microwave background anisotropy power spectrum statistics for high precision cosmology
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