Fig. 11
Ks-band image of the 1.4′ × 1.4′ field centred on the galaxy cluster, as in Figs. 1 and 8, the green contours showing the fluxes of the sources detected at 5σ or more in the MIPS 24 μm image. The red arrows show the positions of red (Y − Ks > 2) galaxies with rising IRAC fluxes ([5.8] − [8.0] > 0), suggesting the possible presence of obscured AGN activity.
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