activity
20182022
most citedThe Aemulus Project I: Numerical Simulations for Precision Cosmology

140 citations · 484 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2022★ 59 cited

The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies

Zhongxu Zhai, Jeremy L. Tinker, Arka Banerjee +6

We analyze clustering measurements of BOSS galaxies using a simulation-based emulator of two-point statistics. We focus on the monopole and quadrupole of the redshift-space correla…

astro-ph.GA2020★ 8 cited

Searching for Dwarf Galaxies in DR2 Phase-Space Data Using Wavelet Transforms

Elise Darragh-Ford, Ethan O. Nadler, Sean McLaughlin +1

We present a wavelet-based algorithm to identify dwarf galaxies in the Milky Way in DR2 data. Our algorithm detects overdensities in 4D position--proper motion space,…

astro-ph.CO2019★ 18 cited

The Aemulus Project IV: Emulating Halo Bias

Thomas McClintock, Eduardo Rozo, Arka Banerjee +6

Models of the spatial distribution of dark matter halos must achieve new levels of precision and accuracy in order to satisfy the requirements of upcoming experiments. In this work…

astro-ph.CO2018★ 131 cited

The Aemulus Project III: Emulation of the Galaxy Correlation Function

Zhongxu Zhai, Jeremy L. Tinker, Matthew R. Becker +6

Using the N-body simulations of the AEMULUS Project, we construct an emulator for the non-linear clustering of galaxies in real and redshift space. We construct our model of galaxy…

astro-ph.CO2018★ 128 cited

The Aemulus Project II: Emulating the Halo Mass Function

Thomas McClintock, Eduardo Rozo, Matthew R. Becker +6

Existing models for the dependence of the halo mass function on cosmological parameters will become a limiting source of systematic uncertainty for cluster cosmology in the near fu…

astro-ph.CO2018★ 140 cited

The Aemulus Project I: Numerical Simulations for Precision Cosmology

Joseph DeRose, Risa H. Wechsler, Jeremy L. Tinker +6

The rapidly growing statistical precision of galaxy surveys has lead to a need for ever-more precise predictions of the observables used to constrain cosmological and galaxy format…