Median SFR values for all three galaxy populations (star-forming, transitioning, and passive) as a function of the tSZ y parameter (left panel). Distribution of the median SFR weighted by the fraction of galaxy density of a given population with respect to the total as a function of the tSZ y parameter (right panel). In both panels, error bars indicate the 68% distribution around the median. Vertical solid lines correspond to the tSZ outer (y_outer = 2.2 × 10⁻⁶) and inner (y_inner = 1.1 × 10⁻⁵) contours. Vertical dashed lines represent y values at which the slopes of the SFR-tSZ relation significantly change (see text).