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This article has an erratum: [https://doi.org/10.1051/0004-6361/202451943e]


Fig. E.2.

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5 σ contrast limits (left) and mass sensitivity (right) for the F480M observations. We show both PCA-roll and TRAP (Samland et al. 2021) contrast limits and convert them into masses with a range of evolutionary models. The uncertainty on the mass sensitivity is propagated based on the uncertainty of the host star.

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