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TOPoS: VI. The metal-weak tail of the metallicity distribution functions of the Milky Way and the Gaia-Sausage-Enceladus structure (Corrigendum).

Authors :
Bonifacio, P.
Monaco, L.
Salvadori, S.
Caffau, E.
Spite, M.
Sbordone, L.
Spite, F.
Ludwig, H.-G.
Di Matteo, P.
Haywood, M.
François, P.
Koch-Hansen, A. J.
Christlieb, N.
Zaggia, S.
Source :
Astronomy & Astrophysics / Astronomie et Astrophysique; 9/29/2022, Vol. 666, p1-1, 1p
Publication Year :
2022

Abstract

Keywords: stars: Population II; stars: abundances; Galaxy: abundances; Galaxy: halo; errata, addenda EN stars: Population II stars: abundances Galaxy: abundances Galaxy: halo errata, addenda 1 1 1 10/03/22 20220929 NES 220929 We realised that there was a mistake in the code that computed parameters for the photometric data sample. Furthermore, for 301 763 stars, the interpolation arrived at the edge in metallicity of the synthetic grid (+0.5) and the program was not extrapolating. Stars: Population II, stars: abundances, Galaxy: abundances, Galaxy: halo, errata, addenda. [Extracted from the article]

Details

Language :
English
ISSN :
00046361
Volume :
666
Database :
Complementary Index
Journal :
Astronomy & Astrophysics / Astronomie et Astrophysique
Publication Type :
Academic Journal
Accession number :
159417579
Full Text :
https://doi.org/10.1051/0004-6361/202140816e