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Karsten Danzmann

Researcher at Leibniz University of Hanover

Publications -  771
Citations -  97810

Karsten Danzmann is an academic researcher from Leibniz University of Hanover. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 112, co-authored 754 publications receiving 80032 citations. Previous affiliations of Karsten Danzmann include Eötvös Loránd University & University of the Balearic Islands.

Papers
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First long-term application of squeezed states of light in a gravitational-wave observatory.

TL;DR: Three new techniques are introduced to enable the long-term application of squeezed light, capable of increasing the astrophysical reach of gravitational-wave detectors, and it is shown that the glitch rate of the detector did not increase from squeezing application.
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Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

Richard J. Abbott, +1338 more
- 31 Jan 2021 - 
TL;DR: The data recorded by these instruments during their first and second observing runs are described, including the gravitational-wave strain arrays, released as time series sampled at 16384 Hz.
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The third generation of gravitational wave observatories and their science reach

M. Punturo, +133 more
TL;DR: The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, is reported in this paper, where an overview of the possible science reaches and the technological progress needed to realize a third generation observatory are discussed.
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GW150914: implications for the stochastic gravitational wave background from binary black holes

B. P. Abbott, +956 more
TL;DR: It is concluded that the stochastic gravitational-wave background from binary black holes, created from the incoherent superposition of all the merging binaries in the Universe, is potentially measurable by the Advanced LIGO and Advanced Virgo detectors operating at their projected final sensitivity.
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Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

B. P. Abbott, +1002 more
TL;DR: The transient noise backgrounds used to determine the significance of the event (designated GW150914) are described and the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of theevent are presented.