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Fig. 7.
Minimal detectable mass with a S/N larger than 10 in one year of LISA observation, as a function of the orbital radius r0. The various Roche limits are those considered in Sect. 5.1. As in Fig. 6, for r0 > 15 M, only the a = 0 curves are shown, the MBH spin playing a negligible role at large distance.
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