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.
Categories: astro-ph.CO