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Fig. 9

image

Median background-subtracted stellar population parameters of UVJ-selected star-forming satellites (open symbols), as a function of distance to the central, in bins of 4′′: stellar mass (top left), extinction (top right), sSFR (bottom left), and sSFR as a fraction of the main-sequence value (assuming a slope of 0.8). Median values for the total distribution of star-forming satellites (i.e., without subtracting the background distribution) are shown in gray, slightly shifted to the left for convenience. Background levels and related uncertainties, estimated at r> 50′′, are shown in green and the virial radius is indicated by a dashed line.

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