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Fig. 16.
Detection-weighted BH-BH merger total intrinsic (not redshifted) mass for models with different assumptions on the pair-instability pulsation supernovae: M70.B (strong PPSN), M60.B (moderate PPSN), M30.B (weak PPSN). For comparison, we also show LIGO/Virgo O1/O2 mean total mass estimates and their 90% confidence limits.
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