  We show that the gravitational waves measurements have raised the opportunity
to measure $H_0$ with dark sirens to within 2$\sigma$, the accuracy required to
resolve the \hubble tension. There are two principal reasons for our results:
(1) upgrades to GW LIGO-Virgo transient catalogues GWTC-1 and GWTC-2 enhance
their sensitive with only 10\% of contamination fraction, and (2) new dark
sirens should help to constrain our dynamical EoS. In conjunction, sensitivity
upgrades and a new dark energy model will facilitate an accurate inference of
the \hubble constant $H_0$ to better with an $\pm 0.077$ error in comparison to
the LIGO dark siren with $+14.0$/$-7.0$, which would further solidify the role
of dark sirens in late dark energy for precision cosmology in the future.
