Figure 16.
Rest-frame colour–magnitude diagrams in NUV − r and g − r for reliable IDs in GAMA, in comparison to the full GAMA sample (grey-scale contours). The thick dashed line in each panel shows the red sequence derived from the GAMA sample in Bourne et al. (2012). Note that H-ATLAS selects galaxies throughout the full locus of GAMA galaxies.

Rest-frame colour–magnitude diagrams in NUV − r and gr for reliable IDs in GAMA, in comparison to the full GAMA sample (grey-scale contours). The thick dashed line in each panel shows the red sequence derived from the GAMA sample in Bourne et al. (2012). Note that H-ATLAS selects galaxies throughout the full locus of GAMA galaxies.

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