Dependence of the COSEBIs saturated information content in form of f for each of the seven parameters while the rest is marginalized over. The above plots are relevant to MS and LS parameters for an angular ranges of  [1′,400′] . The redshift dependence of f is very outstanding here and hence we needed to use logarithmic scales for the y-axes, especially in the cases where cosmic shear analysis is done without any priors.