Showing 1–20 of 23 results
/ Date/ Name
Jun 13, 2016Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914Jun 3, 2016Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceApr 26, 2016Supplement: Localization and broadband follow-up of the gravitational-wave transient GW150914Feb 26, 2016Localization and broadband follow-up of the gravitational-wave transient GW150914Oct 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 eraFeb 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