Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum)

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  • E. P. Bellinger
  • S. Hekker, Max Planck Institute for Solar System Research
  • ,
  • G. C. Angelou, Max Planck Institute for Astrophysics
  • ,
  • A. Stokholm
  • S. Basu, Yale University

The original article presented the density scaling relation (Eq. (2)) incorrectly. The correct relation is: This error affects the rightmost panel of Fig. 10, the bottom left panel of Fig. 13, and the bottom left panel of Fig. 14. The corrected panels are presented in Figs. 1 and 2. The sentence "We note that the large number of outliers in mean density estimates in Fig. 10 arise mainly from their very small uncertainties". is no longer relevant, as the majority of these are no longer outliers with the correct relation.

OriginalsprogEngelsk
ArtikelnummerC2
TidsskriftAstronomy and Astrophysics
Vol/bind635
Antal sider1
ISSN0004-6361
DOI
StatusUdgivet - mar. 2020

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