  The tomography of the polarized Sunyaev-Zeldvich effect due to free electrons
of galaxy clusters can be used to constrain the nature of dark energy because
CMB quadrupoles at different redshifts as the polarization source are sensitive
to the integrated Sachs-Wolfe effect. Here we show that the low multipoles of
the temperature and E-mode polarization anisotropies from the all-sky CMB can
improve the constraint further through the correlation between them and the CMB
quadrupoles viewed from the galaxy clusters. Using a Monte-Carlo simulation, we
find that low multipoles of the temperature and E-mode polarization
anisotropies potentially improve the constraint on the equation of state of
dark energy parameter by $\sim 17$ percent.
