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

Bellinger, E. P., Hekker, S., Angelou, G. C., Stokholm, A., & Basu, S. (2020). Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum). Astronomy and Astrophysics, 635: C2. doi:10.1051/0004-6361/201834461e.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0006-F53F-0 Version Permalink: https://hdl.handle.net/21.11116/0000-0006-F55D-E
Genre: Journal Article

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 Creators:
Bellinger, E. P., Author
Hekker, Saskia1, Author           
Angelou, George C.1, Author           
Stokholm, A., Author
Basu, S., Author
Affiliations:
1Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society, ou_2265636              

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 Dates: 2020
 Publication Status: Published online
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201834461e
 Degree: -

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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: Les Ulis Cedex A France : EDP Sciences
Pages: - Volume / Issue: 635 Sequence Number: C2 Start / End Page: - Identifier: ISSN: 1432-0746
ISSN: 0004-6361
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1