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- W4300158220 abstract "For decades, the determination of the mean density of matter (ΩM) has been tied to the distribution of light. This has led to a bias, perhaps as large as a factor of 2, in determining a key cosmological parameter. Recent measurements of the physical properties of clusters, the cosmic microwave background anisotropy, and the power spectrum of mass inhomogeneity now allow a determination of ΩM without visual bias. The early data lead to a consistent picture of the matter and baryon densities, with ΩB = 0.039 ± 0.0075 and ΩM = 0.33 ± 0.035, respectively." @default.
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- W4300158220 date "2002-09-10" @default.
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- W4300158220 title "The Case for Ω[TINF][ITAL]M[/ITAL][/TINF] = 0.33 ± 0.035" @default.
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- W4300158220 doi "https://doi.org/10.1086/343782" @default.
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