Figure 23: A comparison between the GW amplitude for various sources and the LIGO-II
sensitivity curve based on the analytic estimates from FHH [106]. See the text for details regarding
the computations of . The SNe sources at 10 Mpc; and the Population III sources at a luminosity
distance of 50 Gpc. Secular bar-mode sources are identified with an (s), dynamical bar modes
with a (d). This assumes strong bar modes exist, which has not been demonstrated robustly.
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