Left: HST/ACS F814W images overlaid with H I contours (purple to teal) as in Fig. 1 and CO (1–0) contours (white to red). CO contours correspond to H₂ column densities 2ⁿ × [3.6, 2.6, 2.3, 2.3, 3.9]×10²⁰ cm⁻² (n = 0, 1, 2, …) Center: CHILES Con Pol 1.4 GHz continuum images, overlaid with CO contours (white to dark red). Right: Spitzer 3.6 μm images, converted to bins of stellar mass surface density overlaid with CO contours (black to white). Galaxies are presented in the same order top-to-bottom that they are left-to-right in Figure 1.