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Fig. 4.

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Contour levels at the 68.3% (darker) and 95.4% (lighter) CL of H0 and Ωm in a flat ΛCDM (fΛCDM) model for different cosmological probes: time-delay cosmography in MACS 1149 (r model; blue), Planck (orange), and BAORSD (red). For completeness, we also show the SH0ES measurement of the Hubble parameter (green; Riess et al. 2021). BAORSD includes Gaussian priors on the values of ωb and ns. Details on these datasets are given in Sect. 3.

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