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The Advanced LIGO and Advanced Virgo detectors have enabled the confidentdetection of dozens of mergers of black holes and neutron stars. However, thepresence of detector noise transients (glitches) hinders the search for thesegravitational wave (GW) signals. We prototyped a restructuring of Gravity Spy'sclassification model to distinguish between glitches and astrophysical signals.Our method is able to correctly classify three-quarters of retracted candidateevents in O3b as non-astrophysical and 100\% of the confirmed astrophysicalevents as true signals. This approach will inform candidate event validationefforts in the latest observing run.

A new method to distinguish gravitational-wave signals from detector noise transients with Gravity Spy