Masses and radii for the eclipsing binaries of Table B.2. Blue crosses indicate field stars, while turquoise crosses indicate, from left to right, the low-metallicity globular cluster members NGC 6362 V41 B (Kaluzny et al. 2015), M4 V65 B (Kaluzny et al. 2013), and M55 V54 B (Kaluzny et al. 2014). The red solid line shows our best linear fit. The increasingly darker green dashed lines represent isochrones for 0.2, 2, and 13 Gyr from BHAC15.