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20112026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 37.9k across the 126 of their papers we have counts for

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Showing 2019Show all

12 papers · 1 filter

astro-ph.IM2019★ 4 cited

Geometrical and physical optics analysis for mm-wavelength refractor telescopes designed to map the cosmic microwave background

Jon E. Gudmundsson

We present a compact two-lens HDPE f/1.6 refractor design that is capable of supporting a 28-deg diffraction-limited field of view at 1-mm wavelengths and contrast it to a similar…

astro-ph.IM2019★ 72 cited

PICO: Probe of Inflation and Cosmic Origins

S. Hanany, M. Alvarez, E. Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. W…

astro-ph.IM2019★ 2 cited

CMB-S4 Decadal Survey APC White Paper

Kevork Abazajian, Graeme Addison, Peter Adshead +222

We provide an overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consid…

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.IM2019★ 443 cited

CMB-S4 Science Case, Reference Design, and Project Plan

Kevork Abazajian, Graeme Addison, Peter Adshead +222

We present the science case, reference design, and project plan for the Stage-4 ground-based cosmic microwave background experiment CMB-S4.

astro-ph.CO2019★ 1.1k cited

Planck 2018 results. V. CMB power spectra and likelihoods

Planck Collaboration, N. Aghanim, Y. Akrami +165

This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementin…

astro-ph.CO2019★ 495 cited

Planck 2018 results. VII. Isotropy and Statistics of the CMB

Planck Collaboration, Y. Akrami, M. Ashdown +147

Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with pre…

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★ 54 cited

Primordial Non-Gaussianity

P. Daniel Meerburg, Daniel Green, Muntazir Abidi +175

Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of…

astro-ph.CO2019★ 45 cited

Messengers from the Early Universe: Cosmic Neutrinos and Other Light Relics

Daniel Green, Mustafa A. Amin, Joel Meyers +136

The hot dense environment of the early universe is known to have produced large numbers of baryons, photons, and neutrinos. These extreme conditions may have also produced other lo…

astro-ph.IM2019★ 45 cited

PICO: Probe of Inflation and Cosmic Origins

Shaul Hanany, Marcelo Alvarez, Emmanuel Artis +79

The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce f…

astro-ph.CO2019★ 182 cited

Neutrino physics with the PTOLEMY project: active neutrino properties and the light sterile case

PTOLEMY collaboration, M. G. Betti, M. Biasotti +54

The PTOLEMY project aims to develop a scalable design for a Cosmic Neutrino Background (CNB) detector, the first of its kind and the only one conceived that can look directly at th…