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The prospects for finding transiting exoplanets in the range of a few to 20Earth masses is growing rapidly with both ground-based and spaced-basedefforts. We describe a publicly available computer code to compute and quantifythe compositional ambiguities for differentiated solid exoplanets with ameasured mass and radius, including the mass and radius uncertainties.

A Computational Tool to Interpret the Bulk Composition of Solid Exoplanets based on Mass and Radius Measurements