  We use Pantheon Type Ia supernova (SN Ia) apparent magnitude, DES-3yr binned
SN Ia apparent magnitude, Hubble parameter, and baryon acoustic oscillation
measurements to constrain six spatially flat and non-flat cosmological models.
These sets of data provide mutually consistent cosmological constraints in the
six cosmological models we study. A joint analysis of these data sets provides
model-independent estimates of the Hubble constant, $H_0=68.8\pm1.8\ \rm{km \
s^{-1} \ Mpc^{-1}}$, and the non-relativistic matter density parameter,
$\Omega_{\rm m_0}=0.294\pm0.020$. Although the joint constraints prefer mild
dark energy dynamics and a little spatial curvature, they do not rule out dark
energy being a cosmological constant and flat spatial hypersurfaces. We also
add quasar angular size and H II starburst galaxy measurements to the combined
data set and find more restrictive constraints.
