activity
20182021
most citedRedshift-Space Distortions in Lagrangian Perturbation Theory

140 citations · 406 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2021

The Ly forest flux correlation function: a perturbation theory perspective

Shi-Fan Chen, Zvonimir Vlah, Martin White

The Ly forest provides one of the best means of mapping large-scale structure at high redshift, including our tightest constraint on the distance-redshift relation before cosmic…

astro-ph.CO2021

The cosmology dependence of galaxy clustering and lensing from a hybrid -body-perturbation theory model

Nickolas Kokron, Joseph DeRose, Shi-Fan Chen +2

We implement a model for the two-point statistics of biased tracers that combines dark matter dynamics from -body simulations with an analytic Lagrangian bias expansion. Using A…

astro-ph.CO2020140 cited

Redshift-Space Distortions in Lagrangian Perturbation Theory

Shi-Fan Chen, Zvonimir Vlah, Emanuele Castorina +1

We present the one-loop 2-point function of biased tracers in redshift space computed with Lagrangian perturbation theory, including a full resummation of both long-wavelength (inf…

astro-ph.CO2020

Modeling features in the redshift-space halo power spectrum with perturbation theory

Shi-Fan Chen, Zvonimir Vlah, Martin White

We study the ability of perturbative models with effective field theory contributions and infra-red resummation to model the redshift space clustering of biased tracers in models w…

astro-ph.CO2020134 cited

Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory

Shi-Fan Chen, Zvonimir Vlah, Martin White

The peculiar velocities of biased tracers of the cosmic density field contain important information about the growth of large scale structure and generate anisotropy in the observe…

astro-ph.CO2020

Asymptotic expansions for the Large Scale Structure

Shi-Fan Chen, Massimo Pietroni

We explore the deep ultraviolet (that is, short-distance) limit of the power spectrum (PS) and of the correlation function of a cold dark matter dominated Universe. While for large…