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Fig. D.1.

Fig. D.1. Refer to the following caption and surrounding text.

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Stability of the model parameters for the derivatives when varying the weighting scale σ (see Eq. (D.6)). All points have error bars from Jackknifing over light cones. The first two rows correspond to the derivatives with respect to the cosmological parameters and the third one to the model prediction for the given order of the aperture statistics. Blue rings mark the values obtained from theory for the aperture statistics and their derivatives, estimated from finite differences. The agreement between b and the measurement in cSfid (black) is a test of the robustness of the method.

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