activity
20162022
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 582 across the 7 of their papers we have counts for

collaborators

19 papers

astro-ph.CO2022

Cosmic tidal reconstruction in redshift space

Shi-Hui Zang, Hong-Ming Zhu, Marcel Schmittfull +1

The gravitational coupling between large- and small-scale density perturbations leads to anisotropic distortions to the local small-scale matter fluctuations. Such local anisotropi…

astro-ph.CO2020

Modeling Galaxies in Redshift Space at the Field Level

Marcel Schmittfull, Marko Simonović, Mikhail M. Ivanov +2

We develop an analytical forward model based on perturbation theory to predict the redshift-space galaxy overdensity at the field level given a realization of the initial condition…

astro-ph.CO202020 cited

Galaxy Skew-Spectra in Redshift-Space

Marcel Schmittfull, Azadeh Moradinezhad Dizgah

Modern galaxy surveys focus on the galaxy power spectrum or 2-point correlation function to test and constrain cosmological models. Additional information comes from higher-order N…

astro-ph.CO2020

Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections

Oliver H. E. Philcox, Mikhail M. Ivanov, Matias Zaldarriaga +2

Creating accurate and low-noise covariance matrices represents a formidable challenge in modern-day cosmology. We present a formalism to compress arbitrary observables into a small…

astro-ph.CO20198 cited

Rotation method for accelerating multiple-spherical Bessel function integrals against a numerical source function

Zachary Slepian, Yin Li, Marcel Schmittfull +1

A common problem in cosmology is to integrate the product of two or more spherical Bessel functions (sBFs) with different configuration-space arguments against the power spectrum o…

astro-ph.CO2019

Capturing Non-Gaussianity of the Large-Scale Structure with Weighted Skew-Spectra

Azadeh Moradinezhad Dizgah, Hayden Lee, Marcel Schmittfull +1

The forthcoming generation of wide-field galaxy surveys will probe larger volumes and galaxy densities, thus allowing for a much larger signal-to-noise ratio for higher-order clust…