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Title: Beyond the plane-parallel approximation for redshift surveys

Journal Article · · Monthly Notices of the Royal Astronomical Society
DOI:https://doi.org/10.1093/mnras/sty410· OSTI ID:1461164
 [1]; ORCiD logo [1]
  1. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Redshift -space distortions privilege the location of the observer in cosmological redshift surveys, breaking the translational symmetry of the underlying theory. This violation of statistical homogeneity has consequences for the modelling of clustering observables, leading to what are frequently called `wide-angle effects'. We study these effects analytically, computing their signature in the clustering of the multipoles in configuration and Fourier space. We take into account both physical wide-angle contributions as well as the terms generated by the galaxy selection function. Similar considerations also affect the way power spectrum estimators are constructed. We quantify in an analytical way the biases that enter and clarify the relation between what we measure and the underlying theoretical modelling. The presence of an angular window function is also discussed. Motivated by this analysis, we present new estimators for the three dimensional Cartesian power spectrum and bispectrum multipoles written in terms of spherical Fourier-Bessel coefficients. We show how the latter have several interesting properties, allowing in particular a clear separation between angular and radial modes.

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
Grant/Contract Number:
AC02-05CH11231; SC0017860; 1713791
OSTI ID:
1461164
Alternate ID(s):
OSTI ID: 1593675
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 4; Related Information: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 52 works
Citation information provided by
Web of Science

Cited By (9)

The reconstructed power spectrum in the Zeldovich approximation journal September 2019
The redshift-space momentum power spectrum – I. Optimal estimation from peculiar velocity surveys journal May 2019
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel’dovich approximation journal November 2019
nbodykit: An Open-source, Massively Parallel Toolkit for Large-scale Structure journal September 2018
Ingredients for 21 cm Intensity Mapping journal October 2018
Ingredients for 21cm intensity mapping text January 2018
The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys text January 2019
The Reconstructed Power Spectrum in the Zeldovich Approximation text January 2019
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximation text January 2019

Figures / Tables (6)


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