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Y. Nakato

Researcher at California Institute of Technology

Publications -  13
Citations -  66

Y. Nakato is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Cosmic microwave background & Chemistry. The author has an hindex of 2, co-authored 7 publications receiving 11 citations. Previous affiliations of Y. Nakato include University of Minnesota.

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Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole

TL;DR: The Bicep/Keck Array (BK) program targets the degree angular scales, where the power from primordial B-mode polarization is expected to peak, with ever increasing sensitivity and has published the most stringent constraints on inflation to date as discussed by the authors.
Posted ContentDOI

The Latest Constraints on Inflationary B-modes from the BICEP/Keck Telescopes

BICEPKeck Collaboration P.A.R. Ade, +109 more
TL;DR: In this paper , the Bicep/Keck data were used to constrain the tensor-to-scalar ratio of the BK18 data to 0. 009.

A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set

TL;DR: In this article , the authors present a sample-variance-limited measurement of the temperature power spectrum of the cosmic microwave background (CMB) using observations of a ∼1500 × 1.2 GHz field made by SPT-3G in 2018.
Proceedings ArticleDOI

Observing low elevation sky and the CMB Cold Spot with BICEP3 at the South Pole

J. Kang, +92 more
TL;DR: In this paper, a low-elevation observation strategy was developed to extend coverage of the Southern sky at the South Pole, where BICEP3 can quickly achieve degree-scale E-mode measurements over a large area.
Posted Content

Polarization Calibration of the BICEP3 CMB polarimeter at the South Pole

TL;DR: The BICEP3 CMB Polarimeter as discussed by the authors is a small-aperture refracting telescope located at the South Pole and is specifically designed to search for the possible signature of inflationary gravitational waves in the Cosmic Microwave Background (CMB).