Fig. E.2.
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Semimajor axis versus eccentricity of the Solar System planetesimals at the age of 1000 Myr for the isolated case (contours), and if the Solar System left the cluster at an age of 20 Myr (shades). Both distributions are normalized independently to the maximum value with 10 equally-spaced contour levels each. In Fig. 4 (main paper), we present the results of the same simulations but at an age of 226 Myr.
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