Fig. B.1
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Posterior distributions obtained with a modification of the EOS. Red shows results obtained with Gaussian priors. Blue shows results obtained with uniform priors. T1ba! is fixed at 166.1 K and Z1 = 0.02. The black points correspond to the measured J2n by Juno. The black error bars correspond to Juno’s measurements accounting for differential rotation for the J2n.
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