Abundance patterns of D25_6334, the three stars from E24, and Li-rich stars from L18, compared to typical metal-poor stars, which are shown as violin plots. One of the comparison samples is taken from D25, in which abundances were derived consistently with the present study. The other comparison sample was taken from Li et al. (2022), which mostly contains stars with [Fe/H]<−2. Note that Li-rich stars in L18 were reanalyzed by Li et al. (2022), and we used the latter abundance for consistency. Five unevolved Li-rich stars in Li et al. (2018) are shown with filled symbols, and the other more evolved Li-rich stars are shown with open symbols.