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We use all available baryon acoustic oscillation distance measurements andHubble parameter data to constrain the cosmological constant $\Lambda$,dynamical dark energy, and spatial curvature in simple cosmological models. Wefind that the consensus spatially flat $\Lambda$CDM model provides a reasonablefit to the data, but depending on the Hubble constant prior and cosmologicalmodel, it can be a little more than 1$\sigma$ away from the best-fit model,which can favor mild dark energy dynamics or non-flat spatial hypersurfaces.

Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data