Built on

B. A. Reid and M. White, Towards an accurate model of the redshift-space clustering of haloes in the quasi-linear regime , MNRAS 417
Original
1927
Earlier work this paper cites.
L. Guzzo, M. Pierleoni, B. Meneux, E. Branchini, O. Le Fèvre, C. Marinoni et al., A test of the nature of cosmic acceleration using galaxy redshift distortions , Nature 451
Original
1944
Earlier work this paper cites.
J. C. Jackson, A critique of Rees’s theory of primordial gravitational radiation , MNRAS 156
1972
Earlier work this paper cites.
W. L. W. Sargent and E. L. Turner, A statistical method for determining the cosmological density parameter from the redshifts of a complete sample of galaxies , ApJL 212
1977
Earlier work this paper cites.
N. Kaiser, Clustering in real space and in redshift space , MNRAS 227
1987
Earlier work this paper cites.
J. A. Peacock and S. J. Dodds, Reconstructing the Linear Power Spectrum of Cosmological Mass Fluctuations , MNRAS 267
1994
Earlier work this paper cites.
S. Cole, K. B. Fisher and D. H. Weinberg, Fourier Analysis of Redshift Space Distortions and the Determination of Omega , MNRAS 267
1994
Earlier work this paper cites.
M. S. Vogeley, C. Park, M. J. Geller, J. P. Huchra and J. R. Gott, III, Topological analysis of the CfA redshift survey , APJ 420
1994
Earlier work this paper cites.
K. B. Fisher, On the Validity of the Streaming Model for the Redshift-Space Correlation Function in the Linear Regime , APJ 448
1995
Earlier work this paper cites.
W. E. Ballinger, J. A. Peacock and A. F. Heavens, Measuring the cosmological constant with redshift surveys , MNRAS 282
1996
Earlier work this paper cites.
A. F. Heavens, S. Matarrese and L. Verde, The non-linear redshift-space power spectrum of galaxies , MNRAS 301
1998
Earlier work this paper cites.
M. White, The redshift-space power spectrum in the halo model , MNRAS 321
2001
Earlier work this paper cites.
U. Seljak, Redshift-space bias and β \beta from the halo model , MNRAS 325
2001
Earlier work this paper cites.
X. Kang, Y. P. Jing, H. J. Mo and G. Börner, An analytical model for the non-linear redshift-space power spectrum , MNRAS 336
2002
Earlier work this paper cites.
R. Scoccimarro, Redshift-space distortions, pairwise velocities, and nonlinearities , Physical Review D 70
2004
Earlier work this paper cites.
E. V. Linder, Cosmic growth history and expansion history , Physical Review D 72
2005
Earlier work this paper cites.
J. L. Tinker, D. H. Weinberg and Z. Zheng, Redshift-space distortions with the halo occupation distribution - I. Numerical simulations , MNRAS 368
2006
Earlier work this paper cites.
J. L. Tinker, Redshift-space distortions with the halo occupation distribution - II. Analytic model , MNRAS 374
2007
Earlier work this paper cites.
T. Matsubara, Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space , Physical Review D 77
Original
2008
Earlier work this paper cites.
T. Matsubara, Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture , Physical Review D 78
Original
2008
Earlier work this paper cites.

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Then

Y.-S. Song, C. G. Sabiu, T. Okumura, M. Oh and E. V. Linder, Cosmological tests using redshift space clustering in BOSS DR11 , JCAP 12
Original
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Later among the works it cites.
T. Ishikawa, T. Totani, T. Nishimichi, R. Takahashi, N. Yoshida and M. Tonegawa, On the systematic errors of cosmological-scale gravity tests using redshift-space distortion: non-linear effects and the halo bias , MNRAS 443
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Later among the works it cites.
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Original
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2018

Hybrid modeling of redshift space distortions

Song, Yong-Seon, Zheng, Yi, Taruya, Atsushi et al.

Understand

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 redshift spaces, accurately modeling redshift-space power spectrum is rather difficult due to the non-perturbative properties of the mapping.
Still, however, a perturbative treatment may be applied to the power spectrum at large-scales, and on top of a careful modeling of the Finger-of-God effect caused by the small-scale random motion, the redshift-space power spectrum can be expressed as a series of expansion which contains the higher-order correlations of density and velocity fields.
In our previous work [JCAP 8 (Aug., 2016) 050], we provide a perturbation-theory inspired model for power spectrum in which the higher-order correlations are evaluated directly from the cosmological $N$-body simulations.

Built on

B. A. Reid and M. White, Towards an accurate model of the redshift-space clustering of haloes in the quasi-linear regime , MNRAS 417
Original
1927
Earlier work this paper cites.
L. Guzzo, M. Pierleoni, B. Meneux, E. Branchini, O. Le Fèvre, C. Marinoni et al., A test of the nature of cosmic acceleration using galaxy redshift distortions , Nature 451
Original
1944
Earlier work this paper cites.
J. C. Jackson, A critique of Rees’s theory of primordial gravitational radiation , MNRAS 156
1972
Earlier work this paper cites.
W. L. W. Sargent and E. L. Turner, A statistical method for determining the cosmological density parameter from the redshifts of a complete sample of galaxies , ApJL 212
1977
Earlier work this paper cites.
N. Kaiser, Clustering in real space and in redshift space , MNRAS 227
1987
Earlier work this paper cites.
J. A. Peacock and S. J. Dodds, Reconstructing the Linear Power Spectrum of Cosmological Mass Fluctuations , MNRAS 267
1994
Earlier work this paper cites.
S. Cole, K. B. Fisher and D. H. Weinberg, Fourier Analysis of Redshift Space Distortions and the Determination of Omega , MNRAS 267
1994
Earlier work this paper cites.
M. S. Vogeley, C. Park, M. J. Geller, J. P. Huchra and J. R. Gott, III, Topological analysis of the CfA redshift survey , APJ 420
1994
Earlier work this paper cites.
K. B. Fisher, On the Validity of the Streaming Model for the Redshift-Space Correlation Function in the Linear Regime , APJ 448
1995
Earlier work this paper cites.
W. E. Ballinger, J. A. Peacock and A. F. Heavens, Measuring the cosmological constant with redshift surveys , MNRAS 282
1996
Earlier work this paper cites.
A. F. Heavens, S. Matarrese and L. Verde, The non-linear redshift-space power spectrum of galaxies , MNRAS 301
1998
Earlier work this paper cites.
M. White, The redshift-space power spectrum in the halo model , MNRAS 321
2001
Earlier work this paper cites.
U. Seljak, Redshift-space bias and β \beta from the halo model , MNRAS 325
2001
Earlier work this paper cites.
X. Kang, Y. P. Jing, H. J. Mo and G. Börner, An analytical model for the non-linear redshift-space power spectrum , MNRAS 336
2002
Earlier work this paper cites.
R. Scoccimarro, Redshift-space distortions, pairwise velocities, and nonlinearities , Physical Review D 70
2004
Earlier work this paper cites.
E. V. Linder, Cosmic growth history and expansion history , Physical Review D 72
2005
Earlier work this paper cites.
J. L. Tinker, D. H. Weinberg and Z. Zheng, Redshift-space distortions with the halo occupation distribution - I. Numerical simulations , MNRAS 368
2006
Earlier work this paper cites.
J. L. Tinker, Redshift-space distortions with the halo occupation distribution - II. Analytic model , MNRAS 374
2007
Earlier work this paper cites.
T. Matsubara, Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space , Physical Review D 77
Original
2008
Earlier work this paper cites.
T. Matsubara, Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture , Physical Review D 78
Original
2008
Earlier work this paper cites.