Showing 1–20 of 22 results
/ Date/ Name
Feb 14, 2025Dark Matter Attenuation Effects: Sensitivity Ceilings for Spin-Dependent and Spin-Independent InteractionsMar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino PhysicsOct 28, 2014Characterization of the LIGO detectors during their sixth science runOct 22, 2014Searching for stochastic gravitational waves using data from the two co-located LIGO Hanford detectorsJul 3, 2014Multimessenger Search for Sources of Gravitational Waves and High-Energy Neutrinos: Results for Initial LIGO-Virgo and IceCubeMar 20, 2014Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010Nov 11, 2013Application of a Hough search for continuous gravitational waves on data from the 5th LIGO science runOct 9, 2013Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectorsOct 9, 2013First Searches for Optical Counterparts to Gravitational-wave Candidate EventsSep 24, 2013A directed search for continuous Gravitational Waves from the Galactic CenterSep 24, 2013Search for long-lived gravitational-wave transients coincident with long gamma-ray burstsSep 16, 2013Gravitational waves from known pulsars: results from the initial detector eraJul 31, 2012Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 dataMay 14, 2012A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007Feb 18, 2011Search for gravitational waves from binary black hole inspiral, merger and ringdownNov 17, 2010Search for Gravitational Wave Bursts from Six MagnetarsJul 22, 2010Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science RunJun 13, 2010First search for gravitational waves from the youngest known neutron starMar 12, 2010Sensitivity to Gravitational Waves from Compact Binary Coalescences Achieved during LIGO's Fifth and Virgo's First Science RunMar 12, 2010Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors