Efficient estimators for power spectrum and bispectrum multipole measurements

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Xie, Yunchen, Zhao, Ruiyang, Gu, Gan, Wang, Xiaoma, Mu, Xiaoyong, Wang, Yuting, Zhao, Gong-Bo, Beutler, Florian, Peacock, John A.
Format: Preprint
Published: 2026
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866915983983116288
author Xie, Yunchen
Zhao, Ruiyang
Gu, Gan
Wang, Xiaoma
Mu, Xiaoyong
Wang, Yuting
Zhao, Gong-Bo
Beutler, Florian
Peacock, John A.
author_facet Xie, Yunchen
Zhao, Ruiyang
Gu, Gan
Wang, Xiaoma
Mu, Xiaoyong
Wang, Yuting
Zhao, Gong-Bo
Beutler, Florian
Peacock, John A.
contents Large galaxy surveys demand fast and scalable estimators for anisotropic clustering statistics beyond the monopole. We present a suite of efficient FFT-based estimators for power-spectrum and bispectrum multipoles, built upon exact conjugation and parity symmetries of spherical-harmonic--weighted Fourier transforms of real fields. These symmetries eliminate redundant magnetic sub-configurations, thereby reducing the computational cost by a factor of 2. For the Yamamoto power-spectrum multipoles, we further decrease the cost of high-order even multipoles by algebraically expressing ${L}_{2n}$ in terms of lower-order Legendre polynomials, thereby measuring modified high-order multipoles using only low-$\ell$ fields with a small and controlled deviation from the traditional definition. We introduce a new TripoSH bispectrum estimator obtained by compressing the Scoccimarro bispectrum along an alternative triangle side, which substantially reduces the FFT scaling for commonly used quadrupole configurations in the large-$k$-bin limit. We also derive an analytic treatment of bispectrum shot noise by integrating spherical-harmonic kernels over the triangle-constrained $k$-space volumes, avoiding additional FFTs or costly spherical-Bessel evaluations and enabling fast and accurate shot-noise subtraction. Based on these optimizations, we also introduce CosmoNPC, an open-source Python package for large-scale-structure clustering measurements.
format Preprint
id arxiv_https___arxiv_org_abs_2605_04864
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Efficient estimators for power spectrum and bispectrum multipole measurements
Xie, Yunchen
Zhao, Ruiyang
Gu, Gan
Wang, Xiaoma
Mu, Xiaoyong
Wang, Yuting
Zhao, Gong-Bo
Beutler, Florian
Peacock, John A.
Cosmology and Nongalactic Astrophysics
Large galaxy surveys demand fast and scalable estimators for anisotropic clustering statistics beyond the monopole. We present a suite of efficient FFT-based estimators for power-spectrum and bispectrum multipoles, built upon exact conjugation and parity symmetries of spherical-harmonic--weighted Fourier transforms of real fields. These symmetries eliminate redundant magnetic sub-configurations, thereby reducing the computational cost by a factor of 2. For the Yamamoto power-spectrum multipoles, we further decrease the cost of high-order even multipoles by algebraically expressing ${L}_{2n}$ in terms of lower-order Legendre polynomials, thereby measuring modified high-order multipoles using only low-$\ell$ fields with a small and controlled deviation from the traditional definition. We introduce a new TripoSH bispectrum estimator obtained by compressing the Scoccimarro bispectrum along an alternative triangle side, which substantially reduces the FFT scaling for commonly used quadrupole configurations in the large-$k$-bin limit. We also derive an analytic treatment of bispectrum shot noise by integrating spherical-harmonic kernels over the triangle-constrained $k$-space volumes, avoiding additional FFTs or costly spherical-Bessel evaluations and enabling fast and accurate shot-noise subtraction. Based on these optimizations, we also introduce CosmoNPC, an open-source Python package for large-scale-structure clustering measurements.
title Efficient estimators for power spectrum and bispectrum multipole measurements
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2605.04864