  We discuss several methods which can be used to distinguish the graviton
resonances of the Randall-Sundrum model from the graviton-like resonances which
may occur in other theories. The Breit-Wigner line shape of the RS graviton is
found to be particularly useful. In particular we show that the "effective"
graviton resonance present in the model of Dvali et al ~can be distinguished
from those of the Randall-Sundrum scenario for a reasonably wide range of model
parameters.
