Figure 29

Figure 29: Left: The same as Figure 26 but for Q = 3, MNS = 1.35M ⊙, and a = 0.75,0.5,0, and − 0.5 with a moderately stiff EOS (EOS HB). Right: The same as the left panel but for Q = 4, a = 0.75, and MNS = 1.35M ⊙ with various EOS. The thin dashed curves show the noise curves for LCGT, advanced LIGO, broadband-designed advanced LIGO, and Einstein telescope (from upper to lower). The figures are taken from [109].