Introduction

PK-WL produces tomographic angular power spectra (Cl) and noise power spectra (Nl) estimates for position-position, position-shear, and shear-shear. PK-WL also produces the mixing matrix for modelling the partial observation of the sky.

The estimates are obtained from the same input products and using a similar methodology; therefore, they all share the same running parameters, and are collected in a single output product.

Product relationships for estimates:

Product relationships for mixing matrices:

The catalogue and mask input products are the outputs of CATRED and VMPZ-ID, respectively.