A detection of a core-collapse supernova signal with an Advanced LIGO andVirgo gravitational-wave detector network will allow us to measureastrophysical parameters of the source. In real advanced gravitational-wavedetector data there are transient noise artifacts that may mimic a truegravitational-wave signal. In this paper, we outline a procedure implemented inthe Supernova Model Evidence Extractor (SMEE) that determines if acore-collapse supernova signal candidate is a noise artefact, arapidly-rotating core-collapse supernova signal, or a neutrino explosionmechanism core-collapse supernova signal. Further to this, we use the latestavailable three-dimensional gravitational-wave core-collapse supernovasimulations, and we outline a new procedure for the rejection of backgroundnoise transients when only one detector is operational. We find the minimum SNRneeded to detect all waveforms is reduced when using three-dimensionalwaveforms as signal models.
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