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Showing results 1 to 16 of 16

Issue DateTitleAuthor(s)Type
2020A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers from the First and Second Gravitational-wave Observing Runs김정리Article
2019All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run김정리Article
2022First joint observation by the underground gravitational-wave detector KAGRA with GEO 600김정리Article
2019First Measurement of the Hubble Constant from a Dark Standard Siren using the Dark Energy Survey Galaxies and the LIGO/Virgo Binary-Black-hole Merger GW170814김정리Article
2020GW190521: A Binary Black Hole Merger with a Total Mass of 150 M-circle dot김정리Article
2020Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant김정리Article
2022Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run김정리Article
2021Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo김정리Article
2021Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog김정리Article
2020Properties and Astrophysical Implications of the 150 M Binary Black Hole Merger GW190521김정리Article
2019Search for gravitational waves from Scorpius X-1 in the second Advanced LIGO observing run with an improved hidden Markov model김정리Article
2019Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo김정리Article
2018Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run김정리Article
2019Search for the isotropic stochastic background using data from Advanced LIGO's second observing run김정리Article
2019Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO김정리Article
2022Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs김정리Article

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