Figure 9: The smallest fraction of black hole mass in ringdown waveforms that is needed to
observe the fundamental mode at a distance of 3 Gpc (left) for three values of the black hole spin,
(solid line) (dashed line) and (dot-dashed line) and the error in the
measurement of the various parameters as a function of the black hole spin for the same mode (right).
Figure reprinted with permission from [78]. Ⓒ The American Physical Society.
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