IR-radio correlation values of the full sample of 11 massive galaxy clusters vs. redshift. Sources with detections in the IR and radio were used to determine the values of q₂₄ (left) and q₁₆₀ (right) that are shown as blue and green points, respectively. Sources that were only detected in the IR are lower limits and are shown as light blue and light green points with upper gray arrows. The error bars were derived from the propagation errors. The dashed sky blue, green, and orange lines indicate representative SFG templates from Rieke et al. (2009) at log(L_IR/L_⊙) = [11.00, 11.25, 11.50] for q₂₄. The dashed red line represents the fiducial q₁₆₀ from Alberts et al. (2020).