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Matt Hilton

Researcher at University of KwaZulu-Natal

Publications -  240
Citations -  16177

Matt Hilton is an academic researcher from University of KwaZulu-Natal. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 66, co-authored 222 publications receiving 13760 citations. Previous affiliations of Matt Hilton include University of Nottingham & Council of Scientific and Industrial Research.

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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.