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- W2967492048 abstract "Redshift-space distortions (RSD) in galaxy redshift surveys generally break both the isotropy and homogeneity of galaxy distribution. While the former aspect is particularly highlighted as a probe of growth of structure induced by gravity, the latter aspect, often quoted as wide-angle RSD but ignored in most of the cases, will become important and critical to account for as increasing the statistical precision in next-generation surveys. However, the impact of wide-angle RSD has been mostly studied using linear perturbation theory. In this paper, employing the Zel'dovich approximation, i.e., first-order Lagrangian perturbation theory for gravitational evolution of matter fluctuations, we present a quasi-linear treatment of wide-angle RSD, and compute the cross-correlation function. The present formalism consistently reproduces linear theory results, and can be easily extended to incorporate relativistic corrections (e.g., gravitational redshift)." @default.
- W2967492048 created "2019-08-22" @default.
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- W2967492048 date "2019-11-23" @default.
- W2967492048 modified "2023-10-16" @default.
- W2967492048 title "Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel’dovich approximation" @default.
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- W2967492048 doi "https://doi.org/10.1093/mnras/stz3272" @default.
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