Comparison Between $\chi^2$ and Bayesian Statistics with Considering the Redshift Dependence of Stretch and Color from JLA Data

Ze Zhao

Table 1 Cosmology-fits results given by $\chi^2$ statistics and Bayesian statistics for the $\Lambda$CDM model. For each statistical methods, we consider two cases: constant $\alpha$ and $\beta$; linear $\alpha$ and $\beta$. Both the best-fit result and the 1$\sigma$ errors of parameters given by JLA data are listed in this table.