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thumbnail Fig. 9

Univariate posterior distributions of power spectrum amplitudes for a test without (left panel) and with (right panel) foreground corrections over the full range of Fourier modes considered in this work. Red lines correspond to the true underlying cosmological power spectrum from which mock data sets were generated. The left panel clearly shows that uncorrected foreground effects yield excessive power for large-scale modes and also introduce an overall biased result. In contrast, the right panel shows results obtained from our test with foreground corrections. Clearly, a detailed treatment of all foreground effects permits us to obtain an unbiased measurement of power spectrum amplitudes over the full range of Fourier modes.

Open with DEXTER
In the text
Australia Bust Waist Hips
CM Inches CM Inches CM Inches
6 80.5 31.75 62.5 24.75 89.5 35.25
8 83 32.75 65 25.75 92 36.25
10 88 34.75 70 27.75 97 38.25
12 93 36.75 75 29.75 102 40.25
14 98 38.75 80 31.75 107 42.25
16 103 40.75 85 33.75 112 44.25
18 108 42.75 90 35.75 117 46.25
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