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Using some of the latest cosmological data sets publicly available, we derive the strongest bounds in the literature on the sum of the three active neutrino masses, M_, within the assumption of a background flat cosmology. In the most conservative scheme, combining Planck cosmic microwave background temperature anisotropies and baryon acoustic oscillations (BAO) data, as well as the up-to-date constraint on the optical depth to reionization (), the tightest 95% confidence level upper bound we find is M_0. 06 eV from oscillations data would raise the quoted upper bounds by O (0. 1) and would not affect our conclusions.
Vagnozzi et al. (Fri,) studied this question.