VizieR Online Data Catalog: Very metal-poor stars with LAMOST & Subaru. II. (Li+, 2022)

Readers can find more details about the sample and observations in Paper I (Aoki+ 2022, J/ApJ/931/146). The original sample includes 420 objects (with 445 Subaru/HDS spectra; R=36000). In order to obtain sufficient spectral quality to derive the reliable parameters and elemental abundances, spectra with S/N higher than 10 per pixel around 4500Å, or those in which more than 10 FeI lines are detected, have been selected for the following analysis.

(2 data files).