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Adam D. Hincks

Researcher at University of Toronto

Publications -  175
Citations -  15123

Adam D. Hincks is an academic researcher from University of Toronto. The author has contributed to research in topics: Atacama Cosmology Telescope & Cosmic microwave background. The author has an hindex of 62, co-authored 162 publications receiving 12985 citations. Previous affiliations of Adam D. Hincks include Sapienza University of Rome & Pontifical Gregorian University.

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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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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.
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The Atacama Cosmology Telescope: Sunyaev-Zel'dovich selected galaxy clusters at 148 GHz from three seasons of data

Matthew Hasselfield, +56 more
TL;DR: In this paper, the authors presented a catalog of 68 galaxy clusters, of which 19 are new discoveries, detected via the Sunyaev-Zel'dovich effect (SZ) at 148 GHz in the Atacama Cosmology Telescope (ACT) survey on the celestial equator.
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The Atacama Cosmology Telescope: Cosmological Parameters from Three Seasons of Data

Jonathan Sievers, +115 more
TL;DR: In this article, a model of primary cosmological and secondary foreground parameters is fit to the map power spectra and lensing deflection power spectrum, including contributions from both the thermal Sunyaev-Zeldovich (tSZ) effect and the kinematic SZ effect, Poisson and correlated anisotropy from unresolved infrared sources, radio sources and the correlation between the tSZ effect and infrared sources.
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The atacama cosmology telescope: cosmological parameters from the 2008 power spectrum

Jo Dunkley, +84 more
TL;DR: In this paper, the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over 296 deg(exp 2) with the Atacama Cosmology Telescope (ACT) during its 2008 season was analyzed.