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 · 6.6k across the 124 of their papers we have counts for

collaborators
Showing 2016Show all

8 papers · 1 filter

astro-ph.CO2016★ 19 cited

Testing parity-violating physics from cosmic rotation power reconstruction

Toshiya Namikawa

We study the reconstruction of the cosmic rotation power spectrum produced by parity-violating physics, with an eye to ongoing and near future cosmic microwave background (CMB) exp…

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.CO2016★ 47 cited

Testing statistics of the CMB B-mode polarization toward unambiguously establishing quantum fluctuation of vacuum

Maresuke Shiraishi, Chiaki Hikage, Ryo Namba +2

The B-mode polarization in the cosmic microwave background (CMB) anisotropies at large angular scales provides a smoking-gun evidence for the primordial gravitational waves (GWs).…

astro-ph.CO2016★ 39 cited

CMB Lensing Bispectrum from Nonlinear Growth of the Large Scale Structure

Toshiya Namikawa

We discuss detectability of the nonlinear growth of the large-scale structure in the cosmic microwave background (CMB) lensing. Lensing signals involved in CMB anisotropies have be…

astro-ph.CO2016★ 27 cited

Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors

Toshiya Namikawa, Atsushi Nishizawa, Atsushi Taruya

The first discovery of the gravitational wave (GW) event, GW150914, suggests a higher merger rate of black-hole (BH) binaries. If this is true, a number of BH binaries will be obse…

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.CO2016★ 12 cited

Cosmology with the Square Kilometre Array by SKA-Japan

Daisuke Yamauchi, Kiyotomo Ichiki, Kazunori Kohri +8

In the past several decades, the standard cosmological model has been established and its parameters have been measured to a high precision, while there are still many of the funda…