activity
20102026
most citedBICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season

967 citations · 3.8k across the 64 of their papers we have counts for

collaborators
Showing 2016Show all

7 papers · 1 filter

astro-ph.IM2016★ 17 cited

Making maps of Cosmic Microwave Background polarization for B-mode studies: the POLARBEAR example

Davide Poletti, Giulio Fabbian, Maude Le Jeune +46

Analysis of cosmic microwave background (CMB) datasets typically requires some filtering of the raw time-ordered data. Filtering is frequently used to minimize the impact of low fr…

astro-ph.IM2016★ 12 cited

BICEP3 focal plane design and detector performance

H. Hui, P. A. R. Ade, Z. Ahmed +56

BICEP3, the latest telescope in the BICEP/Keck program, started science observations in March 2016. It is a 550mm aperture refractive telescope observing the polarization of the co…

astro-ph.IM2016★ 58 cited

BICEP3 performance overview and planned Keck Array upgrade

J. A. Grayson, P. A. R. Ade, Z. Ahmed +56

BICEP3 is a 520 mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modular…

astro-ph.IM2016★ 7 cited

Optical Characterization of the BICEP3 CMB Polarimeter at the South Pole

K. S. Karkare, P. A. R. Ade, Z. Ahmed +56

BICEP3 is a small-aperture refracting cosmic microwave background (CMB) telescope designed to make sensitive polarization maps in pursuit of a potential B-mode signal from inflatio…

astro-ph.CO2016★ 104 cited

BICEP2 / Keck Array VIII: Measurement of gravitational lensing from large-scale B-mode polarization

The Keck Array, BICEP2 Collaborations, : +63

We present measurements of polarization lensing using the 150 GHz maps which include all data taken by the BICEP2 & Keck Array CMB polarization experiments up to and including the…

astro-ph.IM2016★ 25 cited

BICEP2 / Keck Array VII: Matrix based E/B Separation applied to BICEP2 and the Keck Array

Keck Array, BICEP2 Collaborations, : +63

A linear polarization field on the sphere can be uniquely decomposed into an E-mode and a B-mode component. These two components are analytically defined in terms of spin-2 spheric…