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Dominik Riechers

Researcher at Cornell University

Publications -  313
Citations -  19758

Dominik Riechers is an academic researcher from Cornell University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 70, co-authored 284 publications receiving 16896 citations. Previous affiliations of Dominik Riechers include Max Planck Society & California Institute of Technology.

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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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A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34

Dominik Riechers, +81 more
- 18 Apr 2013 - 
TL;DR: Despite the overall downturn in cosmic star formation towards the highest redshifts, it seems that environments mature enough to form the most massive, intense starbursts existed at least as early as 880 million years after the Big Bang.
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 ArticleDOI

Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission

TL;DR: It is found that nine typical star-forming galaxies about one billion years after the Big Bang have thermal emission that is less than 1/12 that of similar systems about two billion years later, and enhanced [C ii] emission relative to the far-infrared continuum, confirming a strong evolution in the properties of the interstellar medium in the early Universe.
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The Interstellar Medium In Galaxies Seen A Billion Years After The Big Bang

TL;DR: In this article, the authors measured the [CII] gas and dust emission in 9 typical (~1-4L*) star-forming galaxies and found that these galaxies have >12x less thermal emission compared with similar systems ~2 billion years later, confirming a strong evolution in the interstellar medium properties in the early universe.