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Corrigendum: Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars (A&A (2021) 645 (A61) DOI: 10.1051/0004-6361/202038891)

par Karinkuzhi, Drisya ;Van Eck, Sophie ;Goriely, Stéphane ;Siess, Lionel ;Jorissen, Alain ;Merle, Thibault ;Escorza Santos, Ana ;Masseron, Thomas
Référence Astronomy & astrophysics, 645, A61
Publication Publié, 2021-01-01

Article révisé par les pairs

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Résumé :

We noticed a typo in Eq. (6), Sect. 7.2 of the original paper: the normalizing factor 1=N was erroneously omitted, though it was included when computing the reduced χ2 listed in Table 1. The correct equation is the following: (Equation presented) where [X=Fe]obs and [X=Fe]mod are the measured and predicted abundances of a given element X, respectively, and σX,obs is the associated uncertainty on the measured abundance; the number of considered elements is N.