Fig. B.1.
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Histogram of the tensions in cosmological parameters between 2PCF and persistent homology measured on 100 individual lines of sight in the Covariance Training Set (blue) and a Gaussian fit to these values (orange). The actual tension we measured in DES-Y1 is shown by the dashed black line. No tension is observed when running our pipeline on the mock data vector constructed from all simulations of the Covariance Training Set, which is about 12× larger.
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