Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.
III Weak transitions from levels a3F(3, 4) (0.02 eV, 0.05 eV), a5F(1-5) (0.81 eV-0.85 eV), a1D(2) (0.90 eV), a3P(0-3) (1.05 eV-1.07 eV) with solar analysis
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Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version
Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.