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The LIGO/Virgo collaboration published the catalogs GWTC-1, GWTC-2.1 andGWTC-3 containing candidate gravitational-wave (GW) events detected during itsruns O1, O2 and O3. These GW events can be possible sites of neutrino emission.In this paper, we present a search for neutrino counterparts of 90 GWcandidates using IceCube DeepCore, the low-energy infill array of the IceCubeNeutrino Observatory. The search is conducted using an unbinned maximumlikelihood method, within a time window of 1000 s and uses the spatial andtiming information from the GW events. The neutrinos used for the search haveenergies ranging from a few GeV to several tens of TeV. We do not find anysignificant emission of neutrinos, and place upper limits on the flux and theisotropic-equivalent energy emitted in low-energy neutrinos. We also conduct abinomial test to search for source populations potentially contributing toneutrino emission. We report a non-detection of a significant neutrino-sourcepopulation with this test.

A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/Virgo