Color-magnitude diagrams for clusters, from top to bottom: NGC 6475, Ruprecht 147, NGC 7092, and ASCC 123. From left to right: their respective V vs. (B − V), J vs. (G − J), and K_s vs. (J − K_s) CMDs. The cluster members determined from the pipeline are given by teal circles with their corresponding magnitude and color error bars. The cluster astrometric candidates that were later rejected as cluster members are shown by light blue open circles. RGB stars, if any, are indicated by red circles. The red isochrone is the pipeline selected age, plotted with the fitted cluster E(B − V) and d. This isochrone is plotted without the binary offset. The gray isochrone shows the age, E(B − V), and d as determined by Kharchenko et al. (2013). The blue line is the ZAMS plotted with the fitted cluster E(B − V) and d.