activity
20172026
most citedThe CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations

305 citations · 2.5k across the 92 of their papers we have counts for

collaborators
Showing 2021Show all

12 papers · 1 filter

astro-ph.CO2021★ 42 cited

Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys

Gerrit S. Farren, Oliver H. E. Philcox, Blake D. Sherwin

constraints from galaxy surveys are sourced by the geometric properties of two standardisable rulers: the sound horizon scale, , and the matter-radiation equality scale,…

astro-ph.CO2021★ 91 cited

Precision analysis of the redshift-space galaxy bispectrum

Mikhail M. Ivanov, Oliver H. E. Philcox, Takahiro Nishimichi +3

We study the information content of the angle-averaged (monopole) redshift space galaxy bispectrum. The main novelty of our approach is the use of a systematic tree-level perturbat…

astro-ph.CO2021★ 64 cited

Cosmological constraints without fingers of God

Mikhail M. Ivanov, Oliver H. E. Philcox, Marko Simonović +3

Non-linear redshift-space distortions ("fingers of God") are challenging to model analytically, a fact that limits the applicability of perturbation theory in redshift space as com…

astro-ph.CO2021★ 30 cited

Analytic Gaussian Covariance Matrices for Galaxy -Point Correlation Functions

Jiamin Hou, Robert N. Cahn, Oliver H. E. Philcox +1

We derive analytic covariance matrices for the -Point Correlation Functions (NPCFs) of galaxies in the Gaussian limit. Our results are given for arbitrary and projected onto…

astro-ph.CO2021★ 24 cited

A First Detection of the Connected 4-Point Correlation Function of Galaxies Using the BOSS CMASS Sample

Oliver H. E. Philcox, Jiamin Hou, Zachary Slepian

We present an detection of the non-Gaussian 4-Point Correlation Function (4PCF) using a sample of galaxies from the BOSS CMASS dataset. Our…

astro-ph.CO2021★ 59 cited

Cosmology Without Window Functions: Cubic Estimators for the Galaxy Bispectrum

Oliver H. E. Philcox

When analyzing the galaxy bispectrum measured from spectroscopic surveys, it is imperative to account for the effects of non-uniform survey geometry. Conventionally, this is done b…