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Fig. 10


Correlation coefficient matrices under the input cosmology. Left panel: Gaussian case with θker = 1.2, 2.4, and 4.8 arcmin. Right panel: starlet case with θker = 2, 4, and 8 arcmin. Each of the 3 × 3 blocks corresponds to the correlations between two filter scales. With each block, the S/N bins are [1, 1.5, 2, ..., 5, +[. The data vector by starlet is less correlated.

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