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Table 3.
Summary of the main parameters constrained by cosmic shear data and combinations with galaxy clustering.
Parameter | KiDS-1000 PCℓ | KiDS-1000 PCℓ + SDSS |
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S8 |
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σ8 |
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Ωm |
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Notes. Here, we are considering the 68% C.I. (1σ) MAP+PJ-PHD. It is important to note that σ8 and Ωm are not properly constrained by cosmic shear alone.
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