1σ-contours for all pairs of cosmological parameters considered, marginalised over all other parameters. We have used a photometric redshift uncertainty parameter value σ_ph = 0.05, ten photometric redshift bins for tomography N_zbin = 10, and the most flexible intrinsic alignment and bias model considered in this paper, with over two hundred free parameters (N_K = 7, and N_Z = 7). Orange (light hatched) confidence regions result from using galaxy number density correlations (nn) (excluding the non-linear regime) only, red (dark hatched) regions use ellipticity correlations (ϵϵ) alone, and blue (filled) regions correspond to using all available information including density-ellipticity cross-correlations. For reference, the contours obtained from a pure lensing signal are shown as black lines. Flat priors on cosmological parameters have been applied.