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Ronny Nawrodt

Researcher at University of Jena

Publications -  107
Citations -  10182

Ronny Nawrodt is an academic researcher from University of Jena. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 40, co-authored 106 publications receiving 8505 citations. Previous affiliations of Ronny Nawrodt include University of Adelaide & University of Glasgow.

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The Einstein Telescope: a third-generation gravitational wave observatory

M. Punturo, +134 more
TL;DR: The third-generation ground-based observatory Einstein Telescope (ET) project as discussed by the authors is currently in its design study phase, and it can be seen as the first step in this direction.
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Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

J. Abadie, +722 more
TL;DR: In this paper, Kalogera et al. presented an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo.
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Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

J. Abadie, +709 more
TL;DR: In this article, the authors present an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the Initial and Advanced versions of the ground-based LIGO and Virgo Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters.
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A gravitational wave observatory operating beyond the quantum shot-noise limit

J. Abadie, +614 more
- 11 Sep 2011 - 
TL;DR: In this paper, the authors demonstrate the squeezed-light enhancement of GEO600, which will be the GW observatory operated by the LIGO Scientific Collaboration in its search for GWs for the next 3-4 years.
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Sensitivity studies for third-generation gravitational wave observatories

Stefan Hild, +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.