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Table 1

Observational data used for this work: source, number of giants (defined as log g < 3.2), number of dwarfs (log g ≥ 3.2), method of analysis, spectral resolution, and abundances used.

Source n_giants n_dwarfs Method Spectral resolution Abundances
Placco et al. (2014) (compilation) 335(a) 158 1D LTE 35 000–60 000 C, N, Sr, Ba
Molaro et al. (2023) (compilation) 27 24 1D LTE 32 000–140 000 12C, 13C, Sr, Ba
Israelian et al. (2004) 0 31 1D LTE 35 000–50 000 N, O
Spite et al. (2005) 16(b) 0 1D LTE(c) 47 000 N, O
Lai et al. (2008) 16 12 1D LTE 60 000 C, N, O
Fabbian et al. (2009) 0 43 1D NLTE 60 000 C, O
Norris et al. (2013) 15 6 1D LTE 40 000 O
Zhao et al. (2016) 0 11 1D NLTE 60 000 C, O
Cescutti et al. (2022); François et al. (2024) 41 0 1D LTE 65 000–115 000 Sr, Ba

Notes. (a)An evolutionary correction has been applied to the C abundances (Placco et al. 2014). (b)Only unmixed giants have been selected, using the surface abundance of Li as a diagnostic of the mixing (Spite et al. 2005). (c)Nitrogen and oxygen have been corrected for 3D effects (Spite et al. 2005).

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