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Fig. D.4.


Tomographic ξE/B analysis of DES-SV. Each panel shows ξE (diamonds) and ξB (pluses) for the tomographic redshift bin pair z − ij, corresponding to the correlation between photometric redshift bins i and j (see Sect. 3 for the definition of the redshift bins). The E-modes, ξE, can be compared to the theoretical expectation given by the cosmological parameters listed in Table 1. The B-modes, ξB, can be compared to the null-case (dashed) where, for the auto-correlation cases, the reduced χ2 value for the B-modes being equal to zero is listed. The reduced χ2 and p-value of the full data vector is listed in the lower left.

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