Fig. 5.
Constraints on the structure growth parameter 
for different probe combinations: 3 × 2 pt, KiDS-1000 cosmic shear, BOSS galaxy clustering, cosmic shear with galaxy-galaxy lensing (GGL), and cosmic shear with galaxy clustering. Our fiducial and preferred MAP with PJ-HPD credible interval (solid) can be compared to the standard, but shifted, marginal posterior mode with M-HPD credible intervals (dotted). Our results can also be compared to weak lensing measurements from the literature, which typically quote the mean of the marginal posterior mode with tail credible intervals (dashed).
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