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Fig. 4.

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KiDS-1000 E-mode (upper triangle) and B-mode (lower triangle) pseudo-C measurements with the best-fit model from our cosmological analysis in Sect. 6.1 convolved with the data’s mixing matrix (Eq. (14)). The auto- and cross-angular power spectra have been measured in eight log-spaced bandwidths from 76 ≤  ≤ 1500. The error bars are estimated from the covariance (described in Sect. 3.4), calculated with Flask (Xavier et al. 2016) and Salmo (Joachimi et al. 2021b) simulations. We include the best-fit theory for the pseudo B-modes using Eq. (15) (red line); the amplitude is too small to be distinguishable from the zero line with a reduced χ2 ∼ 1 for a null detection.

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