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Fig. 4.

image

Tension between sound horizon and Hubble constant measured from late-time observations and CMB for the following cosmological models: ΛCDM, ΛCDM + Neff, early DE, wCDM, PEDE-CDM (flatness assumed in all cases). Late-time observations include BAO, type Ia supernovae, and three different absolute distance calibrations from gravitational lensing (H0LiCOW), the cosmic distance ladder with Cepheids (SH0ES) or the TRGB (CCHP).

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