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Fig. 5.

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Contour levels at the 68.3% (darker) and 95.4% (lighter) CL of w and H0 in a flat wCDM (fwCDM) model for different cosmological probes: time-delay cosmography in MACS 1149 (r model; blue), Planck (orange), H0LiCOW (brown), and BAORSD (red). The horizontal dashed line corresponds to models with w = −1, i.e. with a cosmological constant. BAORSD includes Gaussian priors on the values of ωb and ns. Details on these datasets are given in Sect. 3.

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