Fig. 11.
Posterior distribution for the SLACS sample with priors according to Table 4. Orange: inference with the SDSS spectra. Purple: inference with SDSS spectra and VIMOS IFU data set. The posterior of λint, 0 was blinded during the analysis (https://github.com/TDCOSMO/hierarchy_analysis_2020_public/blob/6c293af582c398a5c9de60a51cb0c44432a3c598/SLACS_sample/SLACS_constraints.ipynb).
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