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Fig. 6


Orbital eccentricity marginalized posterior PDFs of each L 98-59 planet. The broader red PDF for each planet corresponds to the MCMC only results representing the eccentricity constraint from the RV data alone. The shallower blue PDFs combine the MCMC results with an additional prior from stability and therefore provides a stronger constraint on each planet’s eccentricity. The shaded regions highlight the 95% confidence intervals. The PDFs are plotted on a logarithmic scale for improved visibility.

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