activity
20002022
most citedBICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season

967 citations · 4.7k across the 47 of their papers we have counts for

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Showing 2019Show all

10 papers · 1 filter

astro-ph.GA2019

An Imprint of the Galactic Magnetic Field in the Diffuse Unpolarized Dust Emission

Brandon S. Hensley, Cheng Zhang, James J. Bock

It is well known that aligned, aspherical dust grains emit polarized radiation and that the degree of polarization depends on the angle between the interstellar magnetic field…

astro-ph.IM2019

Microwave multiplexing on the Keck Array

Ari Cukierman, Zeeshan Ahmed, Shawn Henderson +82

We describe an on-sky demonstration of a microwave-multiplexing readout system in one of the receivers of the Keck Array, a polarimetry experiment observing the cosmic microwave ba…

astro-ph.IM2019

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

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.CO2019

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

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…