Chemical Evolution of R-process Elements in Stars (CERES) - III. Chemical abundances of neutron capture elements from Ba to Eu

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Volume 693 (January 2025)

A&A, 693 (2025) A293

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Table 1

Chemical abundances with uncertainties for our sample of stars.

Star	[FeII/H]	nl(Ba)	A(Ba)	σ(Ba)	[Ba/H]	[Ba/Fe]	...
CES0031–1647	−2.31	3	−0.33	0.06	−2.51	−0.20	...
CES0045–0932	−2.80	3	−1.42	0.03	−3.60	−0.80	...
CES0048–1041	−2.33	3	0.15	0.09	−2.03	0.30	...
CES0055–3345	−2.24	3	0.10	0.06	−2.08	0.16	...
CES0059–4524	−2.26	0					...
CES0102–6143	−2.84	3	−0.29	0.18	−2.47	0.37	...
...	...	...	...	...	...	...	...

Notes. The value “nl(X)” corresponds to the number of measured lines for a given element X. The uncertainty “σ(X)” represents the line-to-line scatter when more than a single line of a given element X is available. The complete table is available in machine readable format at the CDS.

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