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Sebastian Steinlechner

Researcher at Maastricht University

Publications -  303
Citations -  77646

Sebastian Steinlechner is an academic researcher from Maastricht University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 93, co-authored 299 publications receiving 62949 citations. Previous affiliations of Sebastian Steinlechner include Glasgow Caledonian University & Max Planck Society.

Papers
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Journal ArticleDOI

Properties and Astrophysical Implications of the 150 M Binary Black Hole Merger GW190521

Richard J. Abbott, +1332 more
TL;DR: The GW190521 signal is consistent with a binary black hole (BBH) merger source at redshift 0.13-0.30 Gpc-3 yr-1.8 as discussed by the authors.
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Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

Richard J. Abbott, +1337 more
TL;DR: In this article, the population of the 47 compact binary mergers detected with a false-alarm rate 1/yr in the second LIGO-Virgo Gravitational-Wave Transient Catalog, GWTC-2.
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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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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.