Beyond the plane-parallel approximation for redshift surveys
Abstract
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.
- Authors:
-
- Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
- OSTI Identifier:
- 1461164
- Alternate Identifier(s):
- OSTI ID: 1593675
- Grant/Contract Number:
- AC02-05CH11231; SC0017860; 1713791
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 476; Journal Issue: 4; Related Information: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; methods: analytical; methods: observational; cosmological parameters; large-scale structure of Universe; cosmology: theory
Citation Formats
Castorina, Emanuele, and White, Martin. Beyond the plane-parallel approximation for redshift surveys. United States: N. p., 2018.
Web. doi:10.1093/mnras/sty410.
Castorina, Emanuele, & White, Martin. Beyond the plane-parallel approximation for redshift surveys. United States. https://doi.org/10.1093/mnras/sty410
Castorina, Emanuele, and White, Martin. Mon .
"Beyond the plane-parallel approximation for redshift surveys". United States. https://doi.org/10.1093/mnras/sty410. https://www.osti.gov/servlets/purl/1461164.
@article{osti_1461164,
title = {Beyond the plane-parallel approximation for redshift surveys},
author = {Castorina, Emanuele and White, Martin},
abstractNote = {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.},
doi = {10.1093/mnras/sty410},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 4,
volume = 476,
place = {United States},
year = {2018},
month = {2}
}
Web of Science
Figures / Tables:

Works referencing / citing this record:
The reconstructed power spectrum in the Zeldovich approximation
journal, September 2019
- Chen, Shi-Fan; Vlah, Zvonimir; White, Martin
- Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 09
The redshift-space momentum power spectrum – I. Optimal estimation from peculiar velocity surveys
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- Howlett, Cullan
- Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel’dovich approximation
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- Taruya, Atsushi; Saga, Shohei; Breton, Michel-Andrès
- Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 3
nbodykit: An Open-source, Massively Parallel Toolkit for Large-scale Structure
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- Hand, Nick; Feng, Yu; Beutler, Florian
- The Astronomical Journal, Vol. 156, Issue 4
Ingredients for 21 cm Intensity Mapping
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- Villaescusa-Navarro, Francisco; Genel, Shy; Castorina, Emanuele
- The Astrophysical Journal, Vol. 866, Issue 2
Ingredients for 21cm intensity mapping
text, January 2018
- Villaescusa-Navarro, Francisco; Genel, Shy; Castorina, Emanuele
- arXiv
The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
text, January 2019
- Howlett, Cullan
- arXiv
The Reconstructed Power Spectrum in the Zeldovich Approximation
text, January 2019
- Chen, Shi-Fan; Vlah, Zvonimir; White, Martin
- arXiv
Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximation
text, January 2019
- Taruya, Atsushi; Saga, Shohei; Breton, Michel-Andrès
- arXiv
Figures / Tables found in this record: