Comparison of the marginalized cosmological model constraints for the REFLEX II survey with the results from the Planck mission for galaxy clusters (Planck Collaboration XX 2014) as well as with the CMB power spectrum (Planck Collaboration XVI 2014) and with the CMB results from the 9 year WMAP data (Hinshaw et al. 2013). The contour lines give the 1σ and 2σ results for the cluster surveys and WMAP mission and the cross gives the 1σ result from Planck CMB (Planck Collaboration XVI 2014).