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Fig. 13

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LFs for different types of galaxies in different environments: upper left panel shows the least dense environment (D1) and bottom right panel shows the most dense environment (D4). Green solid lines show the LFs for all galaxies; blue dashed lines show the LFs for spiral galaxies; red dotted lines show the LFs for elliptical galaxies. The upper LFs in each panel are the observed LFs that are shifted up two units in logarithmic scale and right by one mag. The lower LFs in each panel are the attenuation-corrected LFs. Filled areas show the 95% confidence regions. The panels D1 to D4 show different global environmental regions: D1 are void regions and D4 are supercluster regions. The LFs have been normalised to the volume of each sample.

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