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Arthur Kosowsky

Researcher at University of Pittsburgh

Publications -  255
Citations -  22748

Arthur Kosowsky is an academic researcher from University of Pittsburgh. The author has contributed to research in topics: Cosmic microwave background & Atacama Cosmology Telescope. The author has an hindex of 75, co-authored 239 publications receiving 19720 citations. Previous affiliations of Arthur Kosowsky include Rutgers University & Fermilab.

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The Simons Observatory : Science goals and forecasts

Peter A. R. Ade, +279 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 mentioned in this paper.
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Statistics of cosmic microwave background polarization

TL;DR: In this article, a formalism for analyzing a full-sky temperature and polarization map of the cosmic microwave background is presented, where temperature maps are analyzed by expanding over the set of spherical harmonics to give multipole moments of the two-point correlation function.
Journal ArticleDOI

A Probe of Primordial Gravity Waves and Vorticity

TL;DR: In this article, a formalism for describing an all-sky map of the polarization of the cosmic microwave background is presented, which allows unambiguous identification of long-wavelength gravity waves or large-scale vortical flows at the time of last scattering.
Journal ArticleDOI

Gravitational radiation from first-order phase transitions.

TL;DR: This work considers the stochastic background of gravity waves produced by first-order cosmological phase transitions from two types of sources: colliding bubbles and hydrodynamic turbulence and finds that the characteristic amplitude of the gravity wavesproduced is comparable to that from bubble collisions.
Posted Content

CMB-S4 Science Book, First Edition

TL;DR: The CMB-S4 project as mentioned in this paper is a ground-based cosmic microwave background (CMB) experiment with superconducting cameras, which will be used for the search for the B-mode polarization signature of primordial gravitational waves and the determination of the number and masses of neutrinos.