Typical dependencies between parameters. From the 1 SSP fits to LBG_46190. Contours show 1σ, 2σ and 3σ confidence levels. The green point with error bars are the best fit 1D values, as given in Table 2. The metallicity is completely unconstrained, whereas the parameters A_V, stellar mass and age are relatively well constrained. There is a slight degeneracy between age and dust, with older ages requiring less dust.