Sources of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>H</mml:mi><mml:mn>0</mml:mn></mml:msub></mml:math> -tension in dark energy scenarios

By focusing on the simple $w\neq-1$ extension to $\Lambda$CDM, we assess which epoch(s) possibly source $H_0$-tension. We consider Cosmic Microwave Background (CMB) data in three possible ways: $i)$ complete CMB data; $ii)$ excluding $l<30$ temperature and polarization likelihoods; $iii)$ imposing early universe priors, that disentangle late time physics. Through a joint analysis with low-redshift supernovae type-Ia gravitationally lensed delay datasets, {and neglecting galaxy clustering Baryonic Acoustic Oscillation (BAO) data}, find inclusion of priors is consistent local estimate $H_0$ while low-$l$+lowE likelihoods mildly relaxes tension. This contrast analyses data. Our implementation contrasting effect different shows information from when decoupled late-times physics could be agreement higher value $H_0$. {We also no evidence for dark energy model using only within Finally BAO redshift ranges perform inverse distance ladder analysis, modifications, being perfectly capable alleviating $H_0$-tension including data, would at odds Ly-$\alpha$ due difference $r_{\rm d}\, vs.\, H_0$ correlation between two datasets.} therefore infer speculate estimates originate modeling late-time analysis. turn recasts as an CMB, instead current early-time vs. perspective.