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20112019
most citedBICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array

663 citations · 1.3k across the 21 of their papers we have counts for

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Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2019★ 23 cited

BICEP2 / Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Dataset

Keck Array, BICEP2 Collaborations, : +76

Precision measurements of cosmic microwave background (CMB) polarization require extreme control of instrumental systematics. In a companion paper we have presented cosmological co…

astro-ph.IM2018

High-Precision Scanning Water Vapor Radiometers for Cosmic Microwave Background Site Characterization and Comparison

D. Barkats, R. Bowens-Rubin, W. H. Clay +7

The compelling science case for the observation of B-mode polarization in the cosmic microwave background (CMB) is driving the CMB community to expand the observed sky fraction, ei…

astro-ph.IM2018★ 12 cited

Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

A. Soliman, P. A. R. Ade, Z. Ahmed +75

BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array…

astro-ph.IM2018★ 1 cited

Ultra-Thin Large-Aperture Vacuum Windows for Millimeter Wavelengths Receivers

Denis Barkats, Marion I. Dierickx, John M. Kovac +75

Targeting faint polarization patterns arising from Primordial Gravitational Waves in the Cosmic Microwave Background requires excellent observational sensitivity. Optical elements…

astro-ph.IM2018★ 1 cited

BICEP Array cryostat and mount design

M. Crumrine, P. A. R. Ade, Z. Ahmed +74

Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style…

astro-ph.IM2018★ 93 cited

BICEP Array: a multi-frequency degree-scale CMB polarimeter

Howard Hui, P. A. R. Ade, Z. Ahmed +75

BICEP Array is the newest multi-frequency instrument in the BICEP/Keck Array program. It is comprised of four 550 mm aperture refractive telescopes observing the polarization of th…

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.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…

astro-ph.IM2016★ 38 cited

Initial Performance of BICEP3: A Degree Angular Scale 95 GHz Band Polarimeter

W. L. K. Wu, P. A. R. Ade, Z. Ahmed +49

BICEP3 is a aperture telescope with cold, on-axis, refractive optics designed to observe at the band from the South Pole. It is the newest member of the BICEP/Kec…

astro-ph.IM2014★ 86 cited

BICEP3: a 95 GHz refracting telescope for degree-scale CMB polarization

Z. Ahmed, M. Amiri, S. J. Benton +29

BICEP3 is a 550 mm-aperture refracting telescope for polarimetry of radiation in the cosmic microwave background at 95 GHz. It adopts the methodology of BICEP1, BICEP2 and the Keck…