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The discoveries of high-energy astrophysical neutrinos by IceCube in 2013 andof gravitational waves by LIGO in 2015 have enabled a new era ofmulti-messenger astronomy. Gravitational waves can identify the merging ofcompact objects such as neutron stars and black holes. These compact mergers,especially neutron star mergers, are potential neutrino sources. We present ananalysis searching for neutrinos from gravitational wave sources reported bythe LIGO Virgo Collaboration (LVC). We use a dedicated transient likelihoodanalysis combining IceCube events with source localizations provided by LVC asspatial priors. We report results for all gravitational wave events from theO1, O2, and O3 observing runs.

A Search for IceCube Neutrinos from the First 33 Detected Gravitational Wave Events