Figure 18
Completeness in the bivariate planes of apparent magnitude and u−r colour (top panels), apparent magnitude and effective surface brightness (middle panels), and apparent magnitude and Sérsic index (bottom panels) for GAMA data after year 1 (left-hand panels), year 2 (middle panels) and year 3 (right-hand panels). Contours show the percentage of galaxies enclosed from out to in, 99, 95, 75, 50 and 5 per cent. Apart from the progression in apparent magnitude over the 3 yr, no other obvious bias is evident.

Completeness in the bivariate planes of apparent magnitude and ur colour (top panels), apparent magnitude and effective surface brightness (middle panels), and apparent magnitude and Sérsic index (bottom panels) for GAMA data after year 1 (left-hand panels), year 2 (middle panels) and year 3 (right-hand panels). Contours show the percentage of galaxies enclosed from out to in, 99, 95, 75, 50 and 5 per cent. Apart from the progression in apparent magnitude over the 3 yr, no other obvious bias is evident.

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