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

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32 papers · 1 filter

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.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…

astro-ph.CO2019★ 13 cited

CMB-S4 forecast on the primordial non-Gaussianity parameter of feature models

Wuhyun Sohn, James Fergusson

We present forecasts on the primordial non-Gaussianity parameter of feature models for the future Cosmic Microwave Background Stage-4 (CMB-S4) experiments. The Fisher…

astro-ph.CO2018★ 2.4k cited

Planck 2018 results. X. Constraints on inflation

Planck Collaboration, Y. Akrami, F. Arroja +173

We report on the implications for cosmic inflation of the 2018 Release of the Planck CMB anisotropy measurements. The results are fully consistent with the two previous Planck cosm…

astro-ph.CO2018★ 1.7k cited

Planck 2018 results. I. Overview and the cosmological legacy of Planck

Planck Collaboration, Y. Akrami, F. Arroja +188

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave…

astro-ph.CO2017★ 14 cited

CMB bounds on tensor-scalar-scalar inflationary correlations

Maresuke Shiraishi, Michele Liguori, James R. Fergusson

The nonlinear interaction between one graviton and two scalars is enhanced in specific inflationary models, potentially leading to distinguishable signatures in the bispectrum of t…

astro-ph.CO2015★ 32 cited

Using inpainting to construct accurate cut-sky CMB estimators

H. F. Gruetjen, J. R. Fergusson, M. Liguori +1

The direct evaluation of manifestly optimal, cut-sky CMB power spectrum and bispectrum estimators is numerically very costly, due to the presence of inverse-covariance filtering op…

astro-ph.CO2015★ 721 cited

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Planck Collaboration, N. Aghanim, M. Arnaud +221

This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlations of CMB data, using the hybrid approach employed previously: pixel-based at $\e…

astro-ph.CO2015★ 281 cited

Planck 2015 results. X. Diffuse component separation: Foreground maps

Planck Collaboration, R. Adam, P. A. R. Ade +236

Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization. In this paper we consider…

astro-ph.CO2015★ 178 cited

Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect

Planck Collaboration, N. Aghanim, M. Arnaud +199

We have constructed all-sky y-maps of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency ch…

astro-ph.CO2015★ 482 cited

Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts

Planck Collaboration, P. A. R. Ade, N. Aghanim +233

We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldov…

astro-ph.CO2015★ 172 cited

Planck 2015 results. XIX. Constraints on primordial magnetic fields

Planck Collaboration, P. A. R. Ade, N. Aghanim +230

We compute and investigate four types of imprint of a stochastic background of primordial magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the impact o…

astro-ph.CO2015★ 87 cited

Planck 2015 results. XVIII. Background geometry & topology

Planck Collaboration, P. A. R. Ade, N. Aghanim +223

Full-sky CMB maps from the 2015 Planck release allow us to detect departures from global isotropy on the largest scales. We present the first searches using CMB polarization for co…

astro-ph.CO2015★ 287 cited

Planck 2015 results. XV. Gravitational lensing

Planck Collaboration, P. A. R. Ade, N. Aghanim +227

We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40 sigma), using temperature and polarization data fro…

astro-ph.CO2014★ 54 cited

Polyspectra searches for sharp oscillatory features in cosmic microwave sky data

J. R. Fergusson, H. F. Gruetjen, E. P. S. Shellard +1

We undertake a thorough search for signatures of sharp oscillatory features in the WMAP9 power spectrum and bispectrum as well as in the Planck power spectrum. For the first time,…

astro-ph.CO2014★ 65 cited

Combining power spectrum and bispectrum measurements to detect oscillatory features

J. R. Fergusson, H. F. Gruetjen, E. P. S. Shellard +1

The simplest inflationary models present us with few observable parameters to discriminate between them. A detection of features in the spectra of primordial density perturbations…

astro-ph.CO2014★ 49 cited

Observed parity-odd CMB temperature bispectrum

Maresuke Shiraishi, Michele Liguori, James R. Fergusson

Parity-odd non-Gaussianities create a variety of temperature bispectra in the cosmic microwave background (CMB), defined in the domain: . Thes…

astro-ph.CO2014★ 26 cited

Efficient optimal non-Gaussian CMB estimators with polarisation

J. R. Fergusson

In this paper we demonstrate an efficient method for including both CMB temperature and polarisation data in optimal non-Gaussian estimators. The method relies on orthogonalising t…

astro-ph.CO2014★ 36 cited

General parity-odd CMB bispectrum estimation

Maresuke Shiraishi, Michele Liguori, James R. Fergusson

We develop a methodology for estimating parity-odd bispectra in the cosmic microwave background (CMB). This is achieved through the extension of the original separable modal method…

astro-ph.CO2013★ 457 cited

Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity

Planck Collaboration, P. A. R. Ade, N. Aghanim +237

The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal bispectrum estimators, sep…

astro-ph.CO2012★ 92 cited

Effects and Detectability of Quasi-Single Field Inflation in the Large-Scale Structure and Cosmic Microwave Background

Emiliano Sefusatti, James R. Fergusson, Xingang Chen +1

Quasi-single field inflation predicts a peculiar momentum dependence in the squeezed limit of the primordial bispectrum which smoothly interpolates between the local and equilatera…