  A detection of a core-collapse supernova signal with an Advanced LIGO and
Virgo gravitational-wave detector network will allow us to measure
astrophysical parameters of the source. In real advanced gravitational-wave
detector data there are transient noise artifacts that may mimic a true
gravitational-wave signal. In this paper, we outline a procedure implemented in
the Supernova Model Evidence Extractor (SMEE) that determines if a
core-collapse supernova signal candidate is a noise artefact, a
rapidly-rotating core-collapse supernova signal, or a neutrino explosion
mechanism core-collapse supernova signal. Further to this, we use the latest
available three-dimensional gravitational-wave core-collapse supernova
simulations, and we outline a new procedure for the rejection of background
noise transients when only one detector is operational. We find the minimum SNR
needed to detect all waveforms is reduced when using three-dimensional
waveforms as signal models.
