# Probing core overshooting using subgiant asteroseismology: The case of KIC10273246
## (Corrigendum)

A. Noll, S. Deheuvels, and J. Ballot

IRAP, Université de Toulouse, CNRS, CNES, UPS, Toulouse, France
e-mail: anoll@irap.omp.eu

A&A 647, A187 (2021), https://doi.org/10.1051/0004-6361/202040055

**Key words.** asteroseismology – convection – stars: evolution – stars: interiors – stars: individual: KIC10273246 – errata, addenda

In Noll et al. (2021), Fig. 8 is not the actual échelle diagram of the best model, and must be replaced with Fig. 1 of the present corrigendum. This has no impact on any result or conclusion of the paper.

## References

Noll, A., Deheuvels, S., & Ballot, J. 2021, A&A, 647, A187

<figure><img src="image_1.png" /><figcaption>**Fig. 1.** Actual échelle diagram of the best model for $\alpha_{ov} = 0.15$, which replaces Fig. 8 of Noll et al. (2021).</figcaption></figure>