Measurements of the cosmological parameters $\Omega_m$, $\Omega_k$,
  $\Omega_\textrm{de}(a)$, $H_0$, and $\sum m_\nu$
  From Baryon Acoustic Oscillation measurements with Sloan Digital Sky Survey
SDSS DR14 galaxies, and the acoustic horizon angle $\theta_*$ measured by the
Planck Collaboration, we obtain $\Omega_m = 0.2724 \pm 0.0047$, and $h + 0.020
\cdot \sum{m_\nu} = 0.7038 \pm 0.0060$, assuming flat space and a cosmological
constant. We combine this result with the 2018 Planck
`TT,TE,EE$+$lowE$+$lensing' analysis, and update a study of $\sum m_\nu$ with
new direct measurements of $\sigma_8$, and obtain $\sum m_\nu = 0.27 \pm 0.08$
eV assuming three nearly degenerate neutrino eigenstates. Measurements are
consistent with $\Omega_k = 0$, and $\Omega_\textrm{de}(a) = \Omega_\Lambda$
constant.
