CPD for NGC 3532 comparing the P_rot reported by D. J. Fritzewski et al. (2021a) and our measurements. The filled red circles show literature P_rot for stars where we obtained a P_rot, while the open red circles show literature P_rot for stars where we did not. The filled blue circles show our 41 newly measured P_rot that disagreed by >15% with the D. J. Fritzewski et al. (2021a) P_rot. Black lines connect our measurements and the D. J. Fritzewski et al. (2021a) periods when our P_rot is shorter. Dashed lines are used for the opposite case. In most cases where the P_rot measurements disagree significantly, we measured a P_rot that is much more rapid than that in D. J. Fritzewski et al. (2021a), suggesting that a fraction of our measurements remain impacted by blending.