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Galaxy And Mass Assembly (GAMA) : the 0 013 < z < 0 1 cosmic spectral energy distribution from 0 1 μm to 1 mm

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Figure

Table 1. Coverage of the GAMA regions by filter, for acommon area in all filters (All), within each GAMA sub-region (G09, G12, G15), or for the three regions combined(GAMA)
Table 2. Data selection process. Column 2 shows the limit above which the sample is entirely free ofany colour bias
Figure 2. The colour distributions for our 11-band data with respect to r band. The various lines show the three selection boundaries discussed in the text withthe thick medium dashed boundary taken as our final 1/VMax limit
Table 3. Various constants required for calculation ofthe luminosity density and energy densities.
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