Fig. 6
Left: L8/LIR vs. distance from the cluster centre. The green, red, and blue points indicate the below, on, and above main-sequence galaxies in Fig. 3. The grey lines indicate the average and the range of L8/LIR for main-sequence galaxies in Elbaz et al. (2011). Right: sSFR divided by that of main-sequence galaxies from Rodighiero et al. (2010). The blue circles and the green triangles indicate galaxies with log L8/LIR <−0.75 and >−0.75. The red crosses indicates galaxies without L15 band detection.
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