Left: median rest-frame U − V and V − J colors, derived from SED modeling, of star-forming satellites (filled circles, colored as a function of distance to the central) and centrals (open circle and gray density histogram). The purple lines show the expected colors of stellar populations models of varying age following a “main-sequence” SFH, assuming E(B − V) < 0.3. Right: median observed B − V and V − r colors of satellites, as a function of distance to the central, compared to the expected colors of a star-forming model (main-sequence SFH, black) and a constant SFR one observed ≥100 Myr after the quenching of star formation (gray). We here include dust extinction with E(B − V) = 0–2. The ellipses show the dispersion of B − V and V − r values in each radial bin.