The Cosmological Effect of CMB/BAO Measurements
  In this paper, the CMB/BAO measurements which cover the 13 redshift data in
the regime $0.106 \leq z \leq 2.34$ are given out. The CMB/BAO samples are
based on the BAO distance ratios $r_{s}(z_d)/D_{V}(z)$ and the CMB acoustic
scales $l_{A}$. It could give out the accelerating behaviors of the
$\Lambda$CDM, $w$CDM and o$\Lambda$CDM models. As the direction of the
degeneracy of $\Omega_{m0}-w$ and $\Omega_{m0}-\Omega_{k0}$ are different for
the CMB/BAO and BAO data, the CMB/BAO data show ability of breaking parameter
degeneracy. Our tightest constraining results is from the
BAO+Planck/BAO+$\Omega_{b}h^2$+$\Omega_{m}h^2$ data which has $\Omega_{m0}$
tension, but doesn't have $H_{0}$ tension with the Planck result. The extending
parameters $w$ and $\Omega_{k0}$ could alleviate the $\Omega_{m0}$ tensions
slightly.
