Showing 1–17 of 17 results
/ Date/ Name
Aug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoJan 3, 2022All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 dataNov 30, 2021All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 dataNov 5, 2021GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing RunSep 24, 2021Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing runJul 29, 2021All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo runMay 27, 2021Constraints on dark photon dark matter using data from LIGO's and Virgo's third observing runMay 13, 2021Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing runDec 23, 2020Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910Dec 22, 2020All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systemsOct 27, 2020Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient CatalogOct 27, 2020GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing RunJan 6, 2020GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$Jan 3, 2020A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers From the First and Second Gravitational-wave Observing RunsDec 25, 2019Open data from the first and second observing runs of Advanced LIGO and Advanced VirgoJun 19, 2019Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo networkOct 16, 2017A gravitational-wave standard siren measurement of the Hubble constant