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This article has an erratum: [https://doi.org/10.1051/0004-6361/201834461e]


Fig. 1.

image

Relative uncertainties of the radii of transiting exoplanets as a function of the relative uncertainty in the radius of their host star. The dashed line shows a one-to-one agreement. The shaded region shows the full range of stellar radii uncertainties determined for the 97 stars examined in this paper. Exoplanet data are taken from the collection by Han et al. (2014).

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