Fig. 8.
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Posterior distributions for a subset of the parameters described in Table 3. Blue: constraints from the eight TDCOSMO-2025 lenses, including JWST kinematic data for RX J1131−1231. Orange: constraints from the TDCOSMO-2025 sample + 11 SLACS lenses with KCWI IFU kinematics data. Pink: constraints from TDCOSMO-2025 + SLACS + SL2S sample. All contours include Ωm constraint coming from the Pantheon+ sample (Scolnic et al. 2022); Brout:2022. Priors are described in Table 3. The posteriors distribution of H0 and λint, 0 were blinded during the analysis. Results in combination with the DES-SN5YR likelihood are very similar (see Table 6) and are not shown for conciseness.
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