Fig. 21.
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Comparison between the two modelling teams for the predicted time delays (un-blinded) as a function of H0 for the three image pairs, in flat ΛCDM cosmology with Ωm = 0.3. Each posterior is the final combined posterior from the two mass-model setups: power-law and composite, including external convergence and stellar kinematics, and assuming λint = 1.
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