Export citation and abstract BibTeX RIS
Due to an error, the numbering of the y-axis of the bottom-most panel in Figure 2 in the published version of this article was incorrect. We present the correct version of the figure here (Figure 1). No results, analysis, or discussion are affected by this change.
Figure 1. Color–magnitude diagrams for the five fields. LFC r' − i' colors are displayed, except in the case of Cl1604, where ACS F606W–F814W colors are used. All confirmed supercluster/cluster members are shown and squares correspond to AGN hosts. Dashed lines indicate the boundaries of our red sequence fits. We can see that a higher fraction of AGNs are on the red sequence in the more evolved structures (Cl1324, RXJ1821, and RXJ1757) than in Cl1604 and Cl0023.
Download figure:
Standard image High-resolution image