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Galaxy and Mass Assembly (GAMA): Optimal Tiling of Dense Surveys with a Multi-Object Spectrograph

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Figure

Figure 1 The radial bias of the simulated annealing algorithm used in the AAT 2dF configure software
Figure 2 The state of the GAMA regions after the first year of data. The plots describe survey redshift completeness inside a circular top-hat kernel with a diameter of 0.14 ◦ This was chosen since it is the angular extent of a 1-Mpc system at z ∼ 0.1 assum
Figure 3 Comparison of different tiling approaches. Simulated annealing (SANN), greedy and dengreedy approaches to tiling are simulated on identical data
Figure 4 The spatial completeness of the GAMA regions after the first year of data. The plots describe survey completeness inside a circular top-hat kernel with a diameter of 2 ◦
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