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We update the ingredients of the Gaussian streaming model (GSM) for the redshift-space clustering of biased tracers using the techniques of Lagrangian perturbation theory, effective field theory (EFT) and a generalized Lagrangian bias expansion.
1927
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astro-ph/9708102
A. J. S. Hamilton, Linear Redshift Distortions: a Review · 1998
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S. Hatton and S. Cole, Estimating β \beta from redshift-space distortions in the 2dF galaxy survey
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V. Desjacques, Baryon acoustic signature in the clustering of density maxima
2008
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2009
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L. Wang, B. Reid, and M. White, An analytic model for redshift-space distortions
2014
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M. White, The Zel’dovich approximation
2014
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V. Assassi, D. Baumann, D. Green, and M. Zaldarriaga, Renormalized halo bias
2014
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2014
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2010
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U. Seljak and P. McDonald, Distribution function approach to redshift space distortions
2011
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2012
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2012
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2012
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M. Musso, A. Paranjape, and R. K. Sheth, Scale-dependent halo bias in the excursion set approach
2012
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K. C. Chan, R. Scoccimarro, and R. K. Sheth, Gravity and large-scale nonlocal bias
2012
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2012
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2014
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S. Tassev, N-point statistics of large-scale structure in the Zel’dovich approximation
2014
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2014
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Z. Vlah, M. White, and A. Aviles, A Lagrangian effective field theory
2015
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T. Matsubara, Recursive Solutions of Lagrangian Perturbation Theory
2015
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2015
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C. Uhlemann, M. Kopp, and T. Haugg, Edgeworth streaming model for redshift space distortions
2015
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2015
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L. Senatore, Bias in the effective field theory of large scale structures
2015
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M. Mirbabayi, F. Schmidt, and M. Zaldarriaga, Biased tracers and time evolution
2015
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2015
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T. Baldauf, V. Desjacques, and U. Seljak, Velocity bias in the distribution of dark matter halos
2015
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L. Senatore and M. Zaldarriaga, The IR-resummed Effective Field Theory of Large Scale Structures
2015
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2015
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2015
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M. White, Reconstruction within the Zeldovich approximation
2015
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2016
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