CPDs for NGC 3532 based on quality classification of the final P_rot measurement reported for each star. Measurements classified as Quality 3 represent our highest-confidence P_rot, where the measured period was consistent across all three TESS cycles. Quality 2 P_rot are measurements that agreed in two TESS cycles, and Quality 1 P_rot were measured in only one cycle, corresponding to the longest P_rot measured in cases where measurements in multiple cycles disagreed. In total, we make new P_rot measurements for 885 stars, all of which are plotted in the bottom-right CPD. The yellow crosses in that CPD correspond to the 228 stars with HDBSCAN membership probabilities of <50% as indicated by E. L. Hunt & S. Reffert (2023) and for which we make new P_rot measurements. Many of these lower-probability members fall on the slow-rotating sequence, suggesting that they are a part of the coeval NGC 3532 population and are likely cluster members.