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Hildebrandt, H., et al. (2017) KiDS-450: Cosmological Parameter Constraints from Tomographic Weak Gravitational Lensing. Monthly Notices of the Royal Astronomical Society, 465, 1454-1498. https://doi.org/10.1093/mnras/stw2805
has been cited by the following article:
TITLE: Measurements of the Cosmological Parameters Ωm and H0
AUTHORS: B. Hoeneisen
KEYWORDS: Cosmological Parameters, Baryon Acoustic Oscillations, Galaxy Distributions, Cosmic Microwave Background
JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.8 No.4, December 29, 2018
ABSTRACT: From Baryon Acoustic Oscillation measurements with Sloan Digital Sky Survey SDSS DR14 galaxies, and the acoustic horizon angle measured by the Planck Collaboration, we obtain Ωm=0.2724±0.0047, and h+0.020⋅∑mv=0.7038±0.0060, assuming flat space and a cosmological constant. We combine this result with the 2018 Planck “TT, TE, EE + lowE + lensing” analysis, and update a study of ∑mv with new direct measurements of σ8, and obtain ∑mv=0.27±0.08 eV assuming three nearly degenerate neutrino eigenstates. Measurements are consistent with Ωk=0, and Ωde(a)=ΩΛ constant.
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