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Andrew Bazarko

Researcher at Princeton University

Publications -  13
Citations -  872

Andrew Bazarko is an academic researcher from Princeton University. The author has contributed to research in topics: Observatory & Telescope. The author has an hindex of 8, co-authored 13 publications receiving 601 citations. Previous affiliations of Andrew Bazarko include Schlumberger.

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Journal ArticleDOI

The Simons Observatory: Science goals and forecasts

Peter A. R. Ade, +248 more
TL;DR: The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s as discussed by the authors.
Journal Article

The Simons Observatory

Adrian T. Lee, +281 more
TL;DR: The Simons Observatory (SO) is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough discoveries in fundamental physics, cosmology, and astrophysics as mentioned in this paper.
Journal Article

The Simons Observatory: Astro2020 Decadal Project Whitepaper

Maximilian H. Abitbol, +281 more
TL;DR: The Simons Observatory (SO) as mentioned in this paper is a ground-based cosmic microwave background (CMB) experiment sited on Cerro Toco in the Atacama Desert in Chile that promises to provide breakthrough discoveries in fundamental physics, cosmology, and astrophysics.
Proceedings ArticleDOI

CCAT-prime: a novel telescope for submillimeter astronomy

TL;DR: The CCAT-prime telescope as discussed by the authors is a 6-meter aperture, crossed-Dragone telescope, designed for millimeter and sub-millimeter wavelength observations, which is located at an altitude of 5600 meters, just below the summit of Cerro Chajnantor in the high Atacama region of Chile.
Journal ArticleDOI

Small Aperture Telescopes for the Simons Observatory

TL;DR: The Simons Observatory (SO) as discussed by the authors is an upcoming cosmic microwave background (CMB) experiment located on Cerro Toco, Chile, that will map the microwave sky in temperature and polarization in six frequency bands spanning 27 to 285 GHz.