activity
20062023
most citedPlanck 2018 results. X. Constraints on inflation

2.4k citations · 8.7k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph.CO2023★ 15 cited

High-resolution CMB bispectrum estimator with flexible modal basis

Wuhyun Sohn, James R. Fergusson, E. P. S. Shellard

We present a new independent pipeline for the CMB bispectrum estimation of primordial non-Gaussianity and release a public code for constraining bispectrum shapes of interest based…

astro-ph.CO2020★ 3 cited

Projected two- and three-point statistics: Forecasts and mitigation of non-linear RSDs

Oliver Leicht, Tobias Baldauf, James Fergusson +1

The combination of two- and three-point clustering statistics of galaxies and the underlying matter distribution has the potential to break degeneracies between cosmological parame…

astro-ph.IM2019★ 79 cited

The Simons Observatory: Astro2020 Decadal Project Whitepaper

The Simons Observatory Collaboration, Maximilian H. Abitbol, Shunsuke Adachi +280

The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough…

astro-ph.CO2019★ 159 cited

Planck 2018 results. IX. Constraints on primordial non-Gaussianity

Planck Collaboration, Y. Akrami, F. Arroja +157

We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare e…

astro-ph.CO2019★ 9 cited

General modal estimation for cross-bispectra

Maresuke Shiraishi, Michele Liguori, James R. Fergusson +1

We describe a fast, optimal estimator for measuring angular bispectra between two correlated weakly non-Gaussian fields ( and ) from observational datasets, based on a separa…

astro-ph.CO2019★ 6 cited

Advancing the matter bispectrum estimation of large-scale structure: a comparison of dark matter codes

Johnathan Hung, James R. Fergusson, E. P. S. Shellard

Cosmological information from forthcoming galaxy surveys, such as LSST and Euclid, will soon exceed that available from the CMB. Higher order correlation functions, like the bispec…