Fig. A.1.
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Corner plots showing the posterior distributions for a simulated galaxy (using a τ-delayed SFH) at redshift 1.89, obtained with the τ-delayed model (left) and Dirichlet model (right). Each posterior uses 500 samples. Kernel density estimation contours are shown with different shades at iso-proportions of the density of samples. The solid lines correspond to the true values.
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