428757.fig.0013
Figure 13: Spectral distributions of GWs from matter motions (“Matter”) and neutrino emission (“Neutrino”) seen from the pole or the equator for a representative 3D rotating model (e.g., [210]) with the expected detection limits of TAMA300 [12], first LIGO and advanced LIGO [218], Large-scale Cryogenic Gravitational wave Telescope (LCGT) [219] and Fabry-Perot type DECIGO [215]. It is noted that is the characteristic gravitational wave strain defined in [220]. The distance to the supernova is assumed to be 10 kpc. Note that for the matter signal, the + mode seen from the polar direction is plotted (from [210]).