activity
20132022
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 2.1k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2022★ 37 cited

The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status

B. Westbrook, P. A. R. Ade, M. Aguilar +90

We present on the status of POLARBEAR-2 A (PB2-A) focal plane fabrication. The PB2-A is the first of three telescopes in the Simon Array (SA), which is an array of three cosmic mic…

astro-ph.IM2022★ 4 cited

Development of epoxy-based millimeter absorber with expanded polystyrenes and carbon black

Yuki Inoue, Masaya Hasegawa, Masashi Hazumi +2

We recently developed and characterized an absorber for millimeter wavelengths. To absorb the millimeter wave efficiently, we need to develop the low reflection and high absorption…

physics.ins-det2020★ 21 cited

Cryogenic suspension design for a kilometer-scale gravitational-wave detector

Takafumi Ushiba, Tomotada Akutsu, Yoichi Aso +43

We report the mirror suspension design for Large-scale Cryogenic Gravitational wave Telescope, KAGRA, during bKAGRA Phase 1. Mirror thermal noise is one of the fundamental noises f…

gr-qc2020★ 9 cited

Overview of KAGRA : KAGRA science

KAGRA Collaboration, T. Akutsu, M. Ando +240

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured a…

physics.ins-det2020★ 16 cited

High Performance Heat Conductor with Small Spring Constant for Cryogenic Applications

Tomohiro Yamada, Takayuki Tomaru, Toshikazu Suzuki +5

We developed a soft and high thermal conductive heat link for cryogenic applications. The measured maximum thermal conductivity was approximately 18500 W/m/K at 10 K. This spring c…

physics.ins-det2019★ 16 cited

An arm length stabilization system for KAGRA and future gravitational-wave detectors

T. Akutsu, M. Ando, K. Arai +198

Modern ground-based gravitational wave (GW) detectors require a complex interferometer configuration with multiple coupled optical cavities. Since achieving the resonances of the a…

astro-ph.CO2019★ 73 cited

A Measurement of the Degree Scale CMB B-mode Angular Power Spectrum with POLARBEAR

S. Adachi, M. A. O. Aguilar Faúndez, K. Arnold +69

We present a measurement of the -mode polarization power spectrum of the cosmic microwave background (CMB) using taken from July 2014 to December 2016 with the POLARBEAR experim…

astro-ph.IM2019★ 13 cited

Application of the independent component analysis to the iKAGRA data

KAGRA Collaboration, T. Akutsu, M. Ando +244

We apply the independent component analysis (ICA) to the real data from a gravitational wave detector for the first time. Specifically we use the iKAGRA data taken in April 2016, a…

gr-qc2018★ 535 cited

KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

T. Akutsu, M. Ando, K. Arai +188

The recent detections of gravitational waves (GWs) reported by LIGO/Virgo collaborations have made significant impact on physics and astronomy. A global network of GW detectors wil…

astro-ph.IM2018★ 24 cited

Improving the absolute accuracy of the gravitational wave detectors by combining the photon pressure and gravity field calibrators

Yuki Inoue, Sadakazu Haino, Nobuyuki Kanda +5

The absolute accuracy of the estimated parameters of gravitational wave sources will be fundamentally limited by the calibration uncertainties of the detectors in upcoming observat…

gr-qc2017★ 86 cited

Construction of KAGRA: an Underground Gravitational Wave Observatory

T. Akutsu, M. Ando, S. Araki +222

Major construction and initial-phase operation of a second-generation gravitational-wave detector KAGRA has been completed. The entire 3-km detector is installed underground in a m…

physics.ins-det2017★ 20 cited

Mirror actuation design for the interferometer control of the KAGRA gravitational wave telescope

Yuta Michimura, Tomofumi Shimoda, Takahiro Miyamoto +36

KAGRA is a 3-km cryogenic interferometric gravitational wave telescope located at an underground site in Japan. In order to achieve its target sensitivity, the relative positions o…

astro-ph.CO2017★ 127 cited

A Measurement of the Cosmic Microwave Background -Mode Polarization Power Spectrum at Sub-Degree Scales from 2 years of POLARBEAR Data

The POLARBEAR Collaboration, P. A. R. Ade, M. Aguilar +79

We report an improved measurement of the cosmic microwave background (CMB) -mode polarization power spectrum with the POLARBEAR experiment at 150 GHz. By adding new data collect…

astro-ph.IM2017★ 60 cited

Performance of a continuously rotating half-wave plate on the POLARBEAR telescope

Satoru Takakura, Mario Aguilar, Yoshiki Akiba +50

A continuously rotating half-wave plate (CRHWP) is a promising tool to improve the sensitivity to large angular scales in cosmic microwave background (CMB) polarization measurement…

astro-ph.IM2016★ 38 cited

POLARBEAR-2: an instrument for CMB polarization measurements

Y. Inoue, P. Ade, Y. Akiba +83

POLARBEAR-2 (PB-2) is a cosmic microwave background (CMB) polarization experiment that will be located in the Atacama highland in Chile at an altitude of 5200 m. Its science goals…

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★ 11 cited

Two-layer anti-reflection coating with mullite and polyimide foam for large-diameter cryogenic infrared filters

Yuki Inoue, Takaho Hamada, Masaya Hasegawa +8

We have developed a novel two-layer anti-reflection (AR) coating method for large-diameter infrared (IR) filters made of alumina, for the use at cryogenic temperatures in millimete…

astro-ph.IM2016★ 41 cited

Millimeter-Wave Broadband Anti-Reflection Coatings Using Laser Ablation of Sub-Wavelength Structures

Tomotake Matsumura, Karl Young, Qi Wen +7

We report on the first use of laser ablation to make sub-millimeter, broad-band, anti-reflection coatings (ARC) based on sub-wavelength structures (SWS) on alumina and sapphire. We…

astro-ph.IM2015★ 163 cited

The POLARBEAR-2 and the Simons Array Experiment

A. Suzuki, P. Ade, Y. Akiba +86

We present an overview of the design and status of the \Pb-2 and the Simons Array experiments. \Pb-2 is a Cosmic Microwave Background polarimetry experiment which aims to character…

physics.ins-det2015

Hidden photon measurements using the long-baseline cavity of laser interferometric gravitational-wave detector

Yuki Inoue, Koji Ishidoshiro

We suggest a new application for the long-baseline and high powered cavities in a laser-interferometric gravitational-wave~(GW) detector to search for WISPs (weakly interacting sub…

astro-ph.CO2015★ 100 cited

POLARBEAR Constraints on Cosmic Birefringence and Primordial Magnetic Fields

POLARBEAR Collaboration, Peter A. R. Ade, Kam Arnold +84

We constrain anisotropic cosmic birefringence using four-point correlations of even-parity -mode and odd-parity -mode polarization in the cosmic microwave background measurem…

astro-ph.IM2015★ 40 cited

Modeling atmospheric emission for CMB ground-based observations

J. Errard, P. A. R. Ade, Y. Akiba +72

Atmosphere is one of the most important noise sources for ground-based cosmic microwave background (CMB) experiments. By increasing optical loading on the detectors, it amplifies t…

astro-ph.IM2014★ 8 cited

Development and characterization of the readout system for POLARBEAR-2

D. Barron, P. A. R. Ade, Y. Akiba +69

POLARBEAR-2 is a next-generation receiver for precision measurements of the polarization of the cosmic microwave background (Cosmic Microwave Background (CMB)). Scheduled to deploy…

astro-ph.CO2014★ 298 cited

A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-Degree Scales with POLARBEAR

The POLARBEAR Collaboration, P. A. R. Ade, Y. Akiba +71

We report a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile. The faint B-mode polarization si…