H-R diagram for the Section 5.5 reference stars and the Table 4 KOIs. M_K(0) are calculated using the Figure 2 linear mapping between M_K(0) and H_K(0) after applying the Section 5.8 systematic correction to H_K(0). KOI labeling is the same as in Figure 16 on the right. Lines show predicted loci for 10 Gyr age solar metallicity stars (- - -) and 3 Gyr age metal-poor stars (-· ·-) from Dartmouth Stellar Evolution models (Dotter et al. 2008). Note the large number of KOI sub-giants.