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An upper limit on the stochastic gravitational-wave background of cosmological originSearch for gravitational waves from binary black hole inspiral, merger, and ringdownEinstein@Home search for periodic gravitational waves in LIGO S4 dataImproved Upper Limits on the Stochastic Gravitational-Wave Background from 2009–2010 LIGO and Virgo DataSearch for Gravitational Waves Associated with γ -ray Bursts Detected by the Interplanetary NetworkConstraints on Cosmic Strings from the LIGO-Virgo Gravitational-Wave DetectorsSearching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectorsObservation of Gravitational Waves from a Binary Black Hole MergerEinstein@Home search for periodic gravitational waves in early S5 LIGO dataFirst cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgroundsSearches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: Results from the second LIGO science runSearch for gravitational waves associated with 39 gamma-ray bursts using data from the second, third, and fourth LIGO runsGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole CoalescenceMeasurement of a low-absorption sample of OH-reduced fused silicaGW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2Beam quality and noise properties of coherently combined ytterbium doped single frequency fiber amplifiers.Simultaneously suppressing frequency and intensity noise in a Nd:YAG nonplanar ring oscillator by means of the current-lock technique.Laser power stabilization for second-generation gravitational wave detectors.Laser beam quality and pointing measurement with an optical resonator.Automatic laser beam characterization of monolithic Nd:YAG nonplanar ring lasers.High power fundamental mode Nd:YAG laser with efficient birefringence compensation.Shot-noise-limited laser power stabilization with a high-power photodiode array.Laser power stabilization using optical ac coupling and its quantum and technical limits.Continuous-wave single-frequency 532 nm laser source emitting 130 W into the fundamental transversal mode.Laser power noise detection at the quantum-noise limit of 32 A photocurrent.Stabilized high-power laser system for the gravitational wave detector advanced LIGO.Novel technique for thermal lens measurement in commonly used optical components.Characterization of optical systems for the ALPS II experiment.Higher-order Laguerre-Gauss modes in (non-) planar four-mirror cavities for future gravitational wave detectors.Shot-noise-limited laser power stabilization for the AEI 10 m Prototype interferometer.Shot-noise-limited laser power stabilization for the AEI 10 m Prototype interferometer: publisher's note.Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black HolesGW150914: The Advanced LIGO Detectors in the Era of First DiscoveriesCalibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceImproved Analysis of GW150914 Using a Fully Spin-Precessing Waveform ModelProperties of the Binary Black Hole Merger GW150914Tests of General Relativity with GW150914The basic physics of the binary black hole merger GW150914
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hulumtues
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B. Willke
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B. Willke
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Benno Willke
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