Median statistics and the Hubble constant
arXiv:1105.5206 · doi:10.1086/662131
Abstract
Following Gott et al. (2001), we use Huchra's final compilation of 553 measurements of the Hubble constant () to determine median statistical constraints on . We find (or ) $\kmsmpc$, where the errors are the 95% statistical and systematic (or statistical) errors. With about two-third more measurements, these results are close to what Gott et al. found a decade ago, with smaller statistical errors and similar systematic errors.
10 pages, 1 figure
References in corpus (7)
- Signals from the Noise: Image Stacking for Quasars in the FIRST Survey
- The Weak Energy Condition and the Expansion History of the Universe
- The expansion field: The value of H_0
- Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy
- Long-term Variability in the Length of the Solar Cycle
- Time and distance constraints on accelerating cosmological models
- Constraints on the DGP Universe Using Observational Hubble parameter
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