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|A||806 Hutterites||.034||Three-quarters dominant|
|B||806 Hutterites||.034||Fully dominant|
|C||2 #x000d7;806 Hutterites||.034||Fully dominant|
|D||806 Hutterites 500 avuncular- pair offspring||.069||Three-quarters dominant|
|E||806 Hutterites 800 cousin-pair offspring||.048||Fully dominant|
|F||806 Hutterites 500 avuncular- pair offspring||.069||Fully dominant|
|G||2 #x000d7;806 Hutterites 1,000 avuncular- pair offspring||.069||Fully dominant|
Foreground templates (top row) and the observed sky completenesses (bottom row) used to generate and analyse the mock catalogue in this work. The upper left panel shows the reddening map derived from the data of Schlegel et al. (1998). The upper right panel is a star map count obtained as detailed in Sect. 3. The lower left panel gives the observed completeness for the mock CMASS survey and the lower right panel for the mock LOW-Z survey. These maps have been generated from SDSS-DR12 data (Eisenstein et al. 2011).
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