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GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the LaserExpand
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GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2.
We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6 UTC byExpand
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GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence.
On August 14, 2017 at 10∶30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of twoExpand
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Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomyExpand
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Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data.
Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history ofExpand
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences.
The LIGO Scientific and Virgo Collaborations have announced the event GW170817, the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutronExpand
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Beta Rebound in Visuomotor Adaptation: Still the Status Quo?
Oscillatory activity is a prominent feature of electromagnetic signals measured from the brain. Among others, beta oscillations (13–30 Hz) have been extensively investigated in the context ofExpand
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Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors.
Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observationalExpand
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Systematic errors in estimation of gravitational-wave candidate significance
We investigate a critical issue in determining the statistical significance of candidate transient gravitationalwave events in a ground-based interferometer network. Given the presence ofExpand
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Fundamentals of the orbit and response for TianQin
TianQin is a space-based laser interferometric gravitational wave detector aimed at detecting gravitational waves at low frequencies (0.1 mHz -- 1 Hz). It is formed by three identical drag-freeExpand
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