TL;DR
This paper introduces a hybrid Fourier basis approach for large-scale galaxy clustering analysis, combining spherical and Cartesian methods to improve cosmological constraints on very large scales.
Contribution
It proposes a novel hybrid basis method that combines spherical and Cartesian Fourier analyses, addressing limitations of previous approaches on large scales.
Findings
Effective in modeling large-scale clustering with spherical modes.
Compatible with likelihood analysis of primordial non-Gaussianity.
Public code Harmonia released for community use.
Abstract
Future precision cosmology from large-scale structure experiments including the Dark Energy Spectroscopic Instrument (DESI) and Euclid will probe wider and deeper cosmic volumes than those covered by previous surveys. The Cartesian power spectrum analysis of anisotropic galaxy clustering based on the Fourier plane wave basis makes a number of assumptions, including the local plane-parallel approximation, that will no longer be valid on very large scales and may degrade cosmological constraints. We propose an approach that utilises a hybrid basis: on the largest scales, clustering statistics are decomposed into spherical Fourier modes which respect the natural geometry of both survey observations and physical effects along the line of sight, such as redshift-space distortions, the Alcock--Paczy\'nsky and light-cone effects; on smaller scales with far more clustering modes, we retain the…
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