Optimal and exact wide-angle power spectrum estimation
Noah Sailer, Kendrick Smith, Yurii Kvasiuk, Alex Laguë, Selim Hotinli
astro-ph.CO
Submitted: 2026-07-06
Comments: 22+21 pages, 3 figures, minimal approximations. Comments welcome!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- Euclid. I. Overview of the Euclid mission
- The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document
- The SPHEREx Satellite Mission
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- Geometric Biases in Power-Spectrum Measurements
- Wide Angle Effects in Future Galaxy Surveys
- Redshift-space distortions with wide angular separations
- Interpreting measurements of the anisotropic galaxy power spectrum
- Wide-Angle Effects in the Power Spectrum Multipoles in Next-Generation Redshift Surveys
- Measuring line-of-sight dependent Fourier-space clustering using FFTs
- Fast Estimators for Redshift-Space Clustering
- Rapid modelling of the redshift-space power spectrum multipoles for a masked density field
- An optimal FFT-based anisotropic power spectrum estimator
- Limits on statistical anisotropy from BOSS DR12 galaxies using bipolar spherical harmonics
- SuperFaB: a fabulous code for Spherical Fourier-Bessel decomposition
- Harmonic analysis of isotropic fields on the sphere with arbitrary masks
- Validation of Spherical Fourier-Bessel power spectrum analysis with lognormal simulations and eBOSS DR16 LRG EZmocks
- The Galaxy Bispectrum in the Spherical Fourier-Bessel Basis
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