Local structure modeled via Λ-Szekeres patches fitted to Cosmicflows-4 data produces a ~0.5 km/s/Mpc upward shift in H0 from Pantheon+ supernovae, increasing the Hubble tension.
Adame et al.,DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations,J
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An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4
Local structure modeled via Λ-Szekeres patches fitted to Cosmicflows-4 data produces a ~0.5 km/s/Mpc upward shift in H0 from Pantheon+ supernovae, increasing the Hubble tension.