\begin{document}$ w< -1 $\end{document} to \begin{document}$ w > -1 $\end{document} for the four parameterized dark energy models. However, these models cannot adequately reconcile the Hubble tension. Notably, we found that phantom-like dark energy with \begin{document}$ w < -1 $\end{document} can achieve the greatest reduction in the Hubble tension to \begin{document}$ 0.1808\sigma $\end{document}. However, AIC analysis indicates that this alleviation is at the cost of high AIC. We also investigated the effect of constructions on the derivative of the equation of state \begin{document}$ {\rm d}w/{\rm d}a $\end{document}, cosmic density parameter, CMB power spectrum \begin{document}$ C^{TT} $\end{document}, and matter spectra \begin{document}$ P(k) $\end{document}. We also found that the Hubble tension may be related to the reionization process."> Can the late dark energy parameterization reconcile the Hubble tension? -
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