activity
19922023
most citedPlanck 2018 results. I. Overview and the cosmological legacy of Planck

1.7k citations · 35.4k across the 340 of their papers we have counts for

collaborators

345 papers

hep-ph2023★ 9 cited

Constraints on the dark sector from electroweak precision observables

B. M. Loizos, X. G. Wang, A. W. Thomas +2

We revisit the Standard Model fit to electroweak precision observables using the latest data and the Particle Data Group value of the mass of the W boson. This analysis is repeated…

astro-ph.CO2023★ 14 cited

The Impact of Anisotropic Redshift Distributions on Angular Clustering

Antón Baleato Lizancos, Martin White

A leading way to constrain physical theories from cosmological observations is to test their predictions for the angular clustering statistics of matter tracers, a technique that i…

astro-ph.CO2023★ 41 cited

Aemulus : Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos

Joseph DeRose, Nickolas Kokron, Arka Banerjee +6

We present the Aemulus simulations: a suite of 150 -body simulations with a mass resolution of $3.51\times 10^{10} \frac{Ω_{cb}}{0.3} ~ h^{-1} M_{\o…

hep-ex2023

A Time Projection Chamber to Search for Feebly Interacting Bosons via Proton Induced Nuclear Reactions

Martin Sevior, Michael Baker, Lindsey Bignell +7

We propose a new Time Projection Chamber particle detector (TPC) to search for the existence of feebly-interacting bosons and to investigate the existence of the X17 boson, propose…

astro-ph.CO2023★ 29 cited

A comparison of template vs. direct model fitting for redshift-space distortions in BOSS

Mark Maus, Shi-Fan Chen, Martin White

The growth of large-scale structure, as revealed in the anisotropic of clustering of galaxies in the low redshift Universe, provides a stringent test of our cosmological model. The…

astro-ph.CO2022★ 26 cited

Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates

Joseph DeRose, Shi-Fan Chen, Nickolas Kokron +1

Numerical simulations in cosmology require trade-offs between volume, resolution and run-time that limit the volume of the Universe that can be simulated, leading to sample varianc…