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• W2016247910 startingPage "A104" @default.
• W2016247910 abstract "We use angular size versus redshift data for galaxy clusters from Bonamente et al. (2006) to place constraints on model parameters of constant and time-evolving dark energy cosmological models. These constraints are compatible with those from other recent data, but are not very restrictive. A joint analysis of the angular size data with more restrictive baryon acoustic oscillation peak length scale and supernova Type Ia apparent magnitude data favors a spatially-flat cosmological model currently dominated by a time-independent cosmological constant but does not exclude time-varying dark energy." @default.
• W2016247910 created "2016-06-24" @default.
• W2016247910 creator A5056689407 @default.
• W2016247910 creator A5062376442 @default.
• W2016247910 date "2012-07-01" @default.
• W2016247910 modified "2023-10-16" @default.
• W2016247910 title "Galaxy cluster angular-size data constraints on dark energy" @default.
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• W2016247910 doi "https://doi.org/10.1051/0004-6361/201117944" @default.
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