about
Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009–2010 LIGO and Virgo DataObservation of Gravitational Waves from a Binary Black Hole MergerGravitational waves from a compact star in a circular, inspiral orbit, in the equatorial plane of a massive, spinning black hole, as observed by LISAThe last three minutes: Issues in gravitational-wave measurements of coalescing compact binariesDetection, measurement, and gravitational radiationDirectional Limits on Persistent Gravitational Waves Using LIGO S5 Science DataUpper Limits on a Stochastic Background of Gravitational WavesThe transient gravitational-wave skySwiftPointing and the Association between Gamma‐Ray Bursts and Gravitational Wave BurstsSwift pointing and gravitational-wave bursts from gamma-ray burst eventsPlans for the LIGO–TAMA joint search for gravitational wave burstsA first comparison of SLOPE and other LIGO burst event trigger generatorsGravEn: software for the simulation of gravitational wave detector network responseObservational constraints on the neutron star mass distributionGravitational radiation from a particle in circular orbit around a black hole. II. Numerical results for the nonrotating caseObserving binary inspiral in gravitational radiation: One interferometerBinary inspiral, gravitational radiation, and cosmology
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description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Lee Samuel Finn
@ast
Lee Samuel Finn
@en
Lee Samuel Finn
@es
Lee Samuel Finn
@nl
type
label
Lee Samuel Finn
@ast
Lee Samuel Finn
@en
Lee Samuel Finn
@es
Lee Samuel Finn
@nl
prefLabel
Lee Samuel Finn
@ast
Lee Samuel Finn
@en
Lee Samuel Finn
@es
Lee Samuel Finn
@nl
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0000-0002-3937-0688