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Fig. 3.

image

Inference on the Hubble constant H0 and sound horizon rs for different models (at fiducial truncation order for models 1–3), with free Ωk, using time-delay lenses, SN Ia, and BAO. While the inferred parameters can change among models and among truncation choices, the relative discrepancy with CMB measurements remains the same. The credibility contours contain 95% of the marginalised posterior probability. The grey point corresponds to the Planck value of H0 and rs and to a flat Universe.

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