activity
20102026
most citedFirst Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475

99 citations · 371 across the 19 of their papers we have counts for

collaborators

20 papers

astro-ph.IM2026

Development and characterization of a millimeter-wave circular polarization observation method using a quarter-wave plate with Simons Array

Kana Sakaguri, Darcy R. Barron, Yuji Chinone +17

We have developed and demonstrated a method for measuring circular polarization at 90 GHz by combining a quarter-wave plate (QWP) and a continuously rotating half-wave plate (HWP).…

astro-ph.IM2026

The Simons Observatory: Commissioning of the Mid-Frequency Small Aperture Telescopes

Kathleen Harrington, Remington Gerras, Nicholas Galitzki +88

The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO Small Aperture Tel…

astro-ph.IM2026

The Simons Observatory: On-sky performance of radio-transparent multi-layer insulation (RT-MLI) using Styroace-II Styrofoam

Samuel Day-Weiss, Nicholas Galitzki, Atsuto Takeuchi +14

We present the on-sky performance of a Radio-Transparent Multi-Layer Insulation filter (RT-MLI) that uses Styroace-II styrofoam to reject ambient thermal radiation from entering a…

astro-ph.CO2025

Constraints on the polarization angle oscillations of the Crab Nebula with the Simons Array and its applications to the search for axion-like particles

Tylor Adkins, Shahed Shayan Arani, Kam Arnold +27

We present a search for polarization oscillation of the Crab Nebula, also known as Tau A, at millimeter wavelengths using observations with the Simons Array, the successor experime…

astro-ph.IM2025

Feedback-Controlled Beam Pattern Measurement Method Using a Power-Variable Calibration Source for Cosmic Microwave Background Telescopes

Haruaki Hirose, Masaya Hasegawa, Daisuke Kaneko +5

We demonstrate a novel beam pattern measurement method for the side lobe characterization of cosmic microwave background telescopes. The method employs a power-variable artificial…

astro-ph.IM2024★ 1 cited

A measurement of atmospheric circular polarization with POLARBEAR

Takuro Fujino, Satoru Takakura, Shahed Shayan Arani +20

At millimeter wavelengths, the atmospheric emission is circularly polarized owing to the Zeeman splitting of molecular oxygen by the Earth's magnetic field. We report a measurement…

astro-ph.IM2024

The Simons Observatory: Design, integration, and testing of the small aperture telescopes

Nicholas Galitzki, Tran Tsan, Jake Spisak +77

The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Ata…

astro-ph.IM2024

A Method of Measuring TES Complex ETF Response in Frequency-domain Multiplexed Readout by Single Sideband Power Modulation

Yu Zhou, Tijmen de Haan, Hiroki Akamatsu +5

The digital frequency domain multiplexing (DfMux) technique is widely used for astrophysical instruments with large detector arrays. Detailed detector characterization is required…

astro-ph.CO2024★ 10 cited

Exploration of the polarization angle variability of the Crab Nebula with POLARBEAR and its application to the search for axion-like particles

Shunsuke Adachi, Tylor Adkins, Carlo Baccigalupi +23

The Crab Nebula, also known as Tau A, is a polarized astronomical source at millimeter wavelengths. It has been used as a stable light source for polarization angle calibration in…

astro-ph.IM2024★ 9 cited

The Simons Observatory: Development and Optical Evaluation of Achromatic Half-Wave Plates

Junna Sugiyama, Tomoki Terasaki, Kana Sakaguri +16

The Simons Observatory (SO) experiment is a cosmic microwave background (CMB) experiment located in the Atacama Desert, Chile. The SO' s small aperture telescopes (SATs) consist of…

astro-ph.IM2023★ 3 cited

Anti-reflection coating with mullite and Duroid for large-diameter cryogenic sapphire and alumina optics

Kana Sakaguri, Masaya Hasegawa, Yuki Sakurai +10

We developed a broadband two-layer anti-reflection (AR) coating for use on a sapphire half-wave plate (HWP) and an alumina infrared (IR) filter for the cosmic microwave background…

astro-ph.IM2015★ 14 cited

Development of readout electronics for POLARBEAR-2 Cosmic Microwave Background experiment

K. Hattori, Y. Akiba, K. Arnold +18

The readout of transition-edge sensor (TES) bolometers with a large multiplexing factor is key for the next generation Cosmic Microwave Background (CMB) experiment, Polarbear-2, ha…

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.CO2013★ 94 cited

Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-correlation with the Cosmic Infrared Background

POLARBEAR Collaboration, P. A. R. Ade, Y. Akiba +73

We reconstruct the gravitational lensing convergence signal from Cosmic Microwave Background (CMB) polarization data taken by the POLARBEAR experiment and cross-correlate it with C…

astro-ph.IM2012★ 52 cited

The bolometric focal plane array of the Polarbear CMB experiment

K. Arnold, P. A. R. Ade, A. E. Anthony +53

The Polarbear Cosmic Microwave Background (CMB) polarization experiment is currently observing from the Atacama Desert in Northern Chile. It will characterize the expected B-mode p…

astro-ph.IM2012★ 62 cited

The QUIET Instrument

QUIET Collaboration, C. Bischoff, A. Brizius +52

The Q/U Imaging ExperimenT (QUIET) is designed to measure polarization in the Cosmic Microwave Background, targeting the imprint of inflationary gravitational waves at large angula…

astro-ph.IM2012

Innovative Demodulation Scheme for Coherent Detectors in CMB Experiments

K. Ishidoshiro, Y. Chinone, M. Hasegawa +3

We propose an innovative demodulation scheme for coherent detectors used in cosmic microwave background polarization experiments. Removal of non-white noise, e.g., narrow-band nois…

astro-ph.CO2011★ 11 cited

Ultra High Energy Cosmology with POLARBEAR

B. Keating, S. Moyerman, D. Boettger +52

Observations of the temperature anisotropy of the Cosmic Microwave Background (CMB) lend support to an inflationary origin of the universe, yet no direct evidence verifying inflati…

astro-ph.IM2011★ 8 cited

Calibration System with Cryogenically-Cooled Loads for CMB Polarization Detectors

M. Hasegawa, O. Tajima, Y. Chinone +3

We present a novel system to calibrate millimeter-wave polarimeters for CMB polarization measurements. This technique is an extension of the conventional metal mirror rotation appr…

astro-ph.CO2010★ 99 cited

First Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475

QUIET Collaboration, C. Bischoff, A. Brizius +48

The Q/U Imaging ExperimenT (QUIET) employs coherent receivers at 43GHz and 95GHz, operating on the Chajnantor plateau in the Atacama Desert in Chile, to measure the anisotropy in t…