“…The distribution of the 51 clones was more widely dispersed than Aurora in a scatter plot of PCOA. Six clones (b‐15, c‐01, c‐02, c‐08, c‐17, and c‐23) whose topcross progenies showed high performance on yields and had been selected for demonstrating the potential of CSS (Tamaki et al, 2009) are marked in Fig. 2 Five of these clones, b‐15, c‐02, c‐08, c‐17, and c‐23, were located far from the 16 individuals of Aurora in the scatter plot by PCOA.…”