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Table 6.

Marginalized posteriors of our hierarchical Bayesian cosmography inference based on the priors and parameterization specified in Table 5 for a flat ΛCDM cosmology.

Data sets H0 [km s−1 Mpc−1] λint, 0 αλ σ(λint) aani σ(aani) σσP, sys
TDCOSMO-only
TDCOSMO+SLACSIFU
TDCOSMO+SLACSSDSS
TDCOSMO+SLACSSDSS + IFU

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