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M

M. Steinke

Researcher at Albert Einstein Institution

Publications -  117
Citations -  53562

M. Steinke is an academic researcher from Albert Einstein Institution. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 64, co-authored 103 publications receiving 43101 citations. Previous affiliations of M. Steinke include Leibniz University of Hanover & Max Planck Society.

Papers
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Journal ArticleDOI

GW150914: First results from the search for binary black hole coalescence with Advanced LIGO

B. P. Abbott, +980 more
- 07 Jun 2016 - 
TL;DR: In this paper, the results of a matched-filter search using relativistic models of compact-object binaries that recovered GW150914 as the most significant event during the coincident observations between the two LIGO detectors were reported.
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The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

B. P. Abbott, +961 more
TL;DR: In this paper, the authors report on the constraints these observations place on the rate of binary black hole coalescences, and estimate a 90% credible range of merger rates between $2$--$53 \, \mathrm{Gpc}^{-3} \mathm{yr}^{ −1}$ (comoving frame).
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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

B. P. Abbott, +1148 more
TL;DR: In this article, the authors presented the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1, during the first and second observing runs of the Advanced Gravitational-wave detector network.
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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.