Figure 13

Figure 13: Distribution of measurement accuracy for a binary merger consisting of two black holes of masses m1 = 106M ⊙ and m2 = 3 × 105M ⊙, based on 10,000 samples of the system in which the sky location and orientation of the binary are chosen randomly. Dashed lines are for nonspinning systems and solid lines are for systems with spin. Figure reprinted with permission from [231].  External LinkThe American Physical Society.