Distance to the main sequence (DMS, eq. 1), or vertical distance between each SFR_Hα (blue) and SFR_IR (orange) marker, and the MS, against clustercentric projected distance. Empty triangles show the population of galaxies with lower (upper) limits in their SFR_Hα (SFR_IR) estimations. Galaxies are color-coded as a function of stellar mass. Galaxies are outlined in different colors in terms of their population: SBGs (blue), MSGs (green), and QINGs (red). Left: Histogram of the DMS for the Hα and mIR detections (blue and orange, respectively), and the Hα and mIR lower (black) and upper (gray) limits. Top: Fraction of QINGs (red), MSGs (green), and SBGs (blue) in distance bins of 0.96r/r₂₀₀ out to 1.25r/r₂₀₀.