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Fig. A.1.


Correlation coefficients of the 3 × 2 pt covariance matrix for the cosmic shear, 𝒞E, galaxy-galaxy lensing, 𝒞nϵ and galaxy clustering observables, ξgg (see Sect. 2 for details). Here the band powers 𝒞, are related to the angular power spectrum C, in Eqs. (1) and (3), as 𝒞 = 2C/(2π).

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