English

Bayesian correction of $H(z)$ data uncertainties

Cosmology and Nongalactic Astrophysics 2018-04-11 v2

Abstract

We compile 41 H(z)H(z) data from literature and use them to constrain OΛ\LambdaCDM and flat Λ\LambdaCDM parameters. We show that the available H(z)H(z) suffers from uncertainties overestimation and propose a Bayesian method to reduce them. As a result of this method, using H(z)H(z) only, we find, in the context of OΛ\LambdaCDM, H0=69.5±2.5kms1Mpc1H_0=69.5\pm2.5\mathrm{\,km\,s^{-1}Mpc^{-1}}, Ωm=0.242±0.036\Omega_m=0.242\pm0.036 and ΩΛ=0.68±0.14\Omega_\Lambda=0.68\pm0.14. In the context of flat Λ\LambdaCDM model, we have found H0=70.4±1.2kms1Mpc1H_0=70.4\pm1.2\mathrm{\,km\,s^{-1}Mpc^{-1}} and Ωm=0.256±0.014\Omega_m=0.256\pm0.014. This corresponds to an uncertainty reduction of up to 30\% when compared to the uncorrected analysis in both cases.

Keywords

Cite

@article{arxiv.1709.00646,
  title  = {Bayesian correction of $H(z)$ data uncertainties},
  author = {J. F. Jesus and T. M. Gregório and F. Andrade-Oliveira and R. Valentim and C. A. O. Matos},
  journal= {arXiv preprint arXiv:1709.00646},
  year   = {2018}
}

Comments

15 pages, 4 figures. New version with a BIC comparison added

R2 v1 2026-06-22T21:31:34.793Z