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Similar

D. W. Pesce et al
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S. Dhawan, D. Brout, D. Scolnic, A. Goobar, A. G. Riess and V. Miranda, arXiv:2001.09260 [astro-ph.CO]
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2020

Is there an early Universe solution to Hubble tension?

Krishnan, Chethan, Colgáin, Eoin Ó, Ruchika et al.

Understand

We consider a low redshift $(z<0.7)$ cosmological dataset comprising megamasers, cosmic chronometers, type Ia SNe and BAO, which we bin according to their redshift.

For each bin, we read the value of $H_0$ by fitting directly to the flat $\Lambda$CDM model.
Doing so, we find that $H_0$ descends with redshift, allowing one to fit a line with a \textit{non-zero} slope of statistical significance $2.1 \, \sigma$.
Our analysis rests on the use of cosmic chronometers to break a degeneracy in BAO data and it will be imperative to revisit this feature as data improves.