We present measurements of Baryon Acoustic Oscillation (BAO) distances used as an uncalibrated standard ruler that determine $\Omega_{\textrm{de}}(a)$, $\Omega_k$, $\Omega_m$, and $d_{\textrm{BAO}} \equiv r_* H_0 / c$; and BAO distances used as a calibrated standard ruler $r_*$ that constrains a combination of $\sum m_\nu$, $h$, and $\Omega_b h^2$. The cosmological parameters obtained in this analysis are compared with the Review of Particle Physics, PDG 2018.