Penton, J.Peyton, J.Zahoor, A.Ratra, B.2026-02-052018Publications of the Astronomical Society of the Pacific, 2018, 130, 993, pp. -46280https://doi.org/10.1088/1538-3873/aadf75https://idr.nitk.ac.in/handle/123456789/24943Zavarygin et al. compiled a list of 15 deuterium abundance measurements; two were discarded because the remaining 13 measurements are then consistent with Gaussianity. Those authors found that the weighted-mean baryon density (?<inf>b</inf>h2) determined from the 13 measurements is mildly discrepant (1.6?) with that determined from the Planck 2015 cosmic microwave background anisotropy data in a flat cosmogony. We find that a median statistic central estimate of ?<inf>b</inf>h2 from all 15 deuterium abundance measurements is a more accurate estimate; is very consistent with ?<inf>b</inf>h2 estimated from Planck 2015 data in a flat cosmogony, but is about 2? lower than that found in a closed cosmogonical model from the Planck 2015 data. © 2018. The Astronomical Society of the Pacific. All rights reserved.(Cosmology:) cosmological parameters(Cosmology:) primordial nucleosynthesisMethods: data analysis