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Nonlinear redshift-space distortion known as the Fingers-of-God (FoG) effect is a major systematic uncertainty in redshift-space distortion studies conducted to test gravity models. The FoG effect has been usually attributed to the random…

宇宙学与河外天体物理 · 物理学 2016-03-28 Chiaki Hikage , Kazuhiro Yamamoto

For decades, cosmologists have been using galaxies to trace the large-scale distribution of matter. At present, the largest source of systematic uncertainty in this analysis is the challenge of modeling the complex relationship between…

宇宙学与河外天体物理 · 物理学 2015-03-19 Chiaki Hikage , Masahiro Takada , David N. Spergel

The complex relationship between the galaxy density field and the underlying matter field limits our ability to extract cosmological constraints from galaxy redshift surveys. Our approach is to use halos rather than galaxies to trace the…

天体物理学 · 物理学 2009-08-12 Beth A. Reid , David N. Spergel , Paul Bode

Inferring line-of-sight distances from redshifts in and around galaxy clusters is complicated by peculiar velocities, a phenomenon known as the "Fingers of God" (FoG). This presents a significant challenge for finding filaments in large…

Future high spectroscopic resolution galaxy surveys will observe galaxies with nearly full-sky footprints. Modeling the galaxy clustering for these surveys, therefore, must include the wide-angle effect with narrow redshift binning. In…

宇宙学与河外天体物理 · 物理学 2020-10-28 Henry S. Grasshorn Gebhardt , Donghui Jeong

Theoretical modeling of the redshift-space power spectrum of galaxies is crucially important to correctly extract cosmological information from redshift surveys. The task is complicated by the nonlinear biasing and redshift space distortion…

宇宙学与河外天体物理 · 物理学 2015-11-26 Teppei Okumura , Nick Hand , Uros Seljak , Zvonimir Vlah , Vincent Desjacques

Non-linear redshift-space distortions ("fingers of God") are challenging to model analytically, a fact that limits the applicability of perturbation theory in redshift space as compared to real space. We show how this problem can be…

宇宙学与河外天体物理 · 物理学 2022-02-24 Mikhail M. Ivanov , Oliver H. E. Philcox , Marko Simonović , Matias Zaldarriaga , Takahiro Nishimichi , Masahiro Takada

Complex radiative transfer (RT) of the Lyman-$\alpha$ photons poses a theoretical challenge to galaxy surveys which infer the large-scale structure with Lyman-$\alpha$ emitters (LAEs). Guided by RT simulations, prior studies investigated…

宇宙学与河外天体物理 · 物理学 2019-09-04 Chris Byrohl , Shun Saito , Christoph Behrens

The mapping of dark matter clustering from real space to redshift space introduces the anisotropic property to the measured density power spectrum in redshift space, known as the redshift space distortion effect. The mapping formula is…

宇宙学与河外天体物理 · 物理学 2016-08-31 Yi Zheng , Yong-Seon Song

It was recently shown that the power spectrum in redshift space can be written as a sum of cross-power spectra between number weighted velocity moments. We investigate the properties of these power spectra for simulated galaxies and dark…

宇宙学与河外天体物理 · 物理学 2015-06-05 Teppei Okumura , Uros Seljak , Vincent Desjacques

The mapping of galaxy clustering from real space to redshift space introduces the anisotropic property to the measured galaxy density power spectrum in redshift space, known as the redshift space distortion (RSD) effect. The mapping formula…

宇宙学与河外天体物理 · 物理学 2019-06-12 Yi Zheng , Yong-Seon Song , Minji Oh

The observed power spectrum in redshift space appears distorted due to the peculiar motion of galaxies, known as redshift-space distortions (RSD). While all the effects in RSD are accounted for by the simple mapping formula from real to…

宇宙学与河外天体物理 · 物理学 2018-07-25 Yong-Seon Song , Yi Zheng , Atsushi Taruya , Minji Oh

Using the galaxy catalog built from ELUCID N-body simulation and the semi-analytical galaxy formation model, we have built a mock HI intensity mapping map. We have implemented the Finger-of-God (FoG) effect in the map by considering the…

宇宙学与河外天体物理 · 物理学 2020-05-25 Jiajun Zhang , André A. Costa , Bin Wang , Jianhua He , Yu Luo , Xiaohu Yang

We investigate the effect of redshift-space distortions in the power spectrum parallel and perpendicular to the observer's line of sight, P(k_par,k_perp), using the optically selected Durham/UKST Galaxy Redshift Survey. On small, non-linear…

天体物理学 · 物理学 2009-10-31 P. J. Outram , Fiona Hoyle , T. Shanks

Large-scale HI surveys and their cross-correlations with galaxy distributions have immense potential as cosmological probes. Interpreting these measurements requires theoretical models that must incorporate redshift-space distortions…

宇宙学与河外天体物理 · 物理学 2025-10-29 Calvin Osinga , Benedikt Diemer , Francisco Villaescusa-Navarro

Intrinsic alignments (IAs) of galaxies/halos observed via galaxy imaging survey, combined with redshift information, offer a novel probe of cosmology as a tracer of the tidal force field of a large-scale structure. In this paper, we present…

宇宙学与河外天体物理 · 物理学 2025-06-03 Atsushi Taruya , Toshiki Kurita , Teppei Okumura

This is the second paper of a series where we study the clustering of LRG galaxies in the latest spectroscopic SDSS data release, DR6, which has 75000 LRG galaxies covering over 1 $Gpc^3/h^3$ for $0.15<z<0.47$. Here we focus on modeling…

天体物理学 · 物理学 2010-11-02 Anna Cabre , Enrique Gaztanaga

Nonlinear redshift-space distortions, the Finger-of-God (FoG) effect, can complicate the interpretation of the galaxy power spectrum. Here, we demonstrate the method proposed by Hikage et al. (2012) to use complimentary observations to…

宇宙学与河外天体物理 · 物理学 2015-06-12 Chiaki Hikage , Rachel Mandelbaum , Masahiro Takada , David N. Spergel

We study the impacts of the satellite galaxies on the redshift-space distortions. In our multipole power spectrum analysis of the luminous red galaxies (LRGs) samples of the Sloan Digital Sky Survey (SDSS), we have clearly detected the…

宇宙学与河外天体物理 · 物理学 2013-09-04 Chiaki Hikage , Kazuhiro Yamamoto

It is generally accepted that linear theory of growth of structure under gravity produces a squashed structure in the two-point correlation function (2PCF) along the line of sight (LoS). On the other hand, the observed radial spread out…

宇宙学与河外天体物理 · 物理学 2019-06-21 Luis Salas , Irene Cruz-González
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