Notes. This catalogue contains all metal-poor entries in the SAGA database. For each NLTE-corrected chemical species X, the table provides: (1) the LTE abundance, [X/H]_LTE; (2) the NLTE correction, d[X/H]_NLTE ≡ [X/H]_NLTE − [X/H]_LTE; (3) the flag OC_X, set to 1 if the abundance was originally published corrected for NLTE effects (in which case d[X/H]_NLTE = 0); (4) the flag OW_X, set to 1 if the abundance was derived using spectral lines not included in our line list (see Table 1, in which case d[X/H]_NLTE = NaN); (5) the flag in grid_X, set to 1 if the star’s stellar parameters fall within the NLTE grid limits, and 0 otherwise; (6) the standard deviation of the average NLTE correction, std_d[X/H]NLTE; and (7) the number of lines used to compute the average correction at the closest grid point to the star, Nl_d[X/H]NLTE (not given for CH and Cu). Additional columns include ‘Line Type’ indicating whether resonance or subordinate lines were used for the Na and Al corrections (not shown here) and ‘C_cor,P’ providing the Placco et al. (2014) evolutionary carbon corrections. Abundance ratios for N, F, Si II, P, S, Ca II, Sc, V, Cr II, Mn II, Ni, Cu II, Zn II, and Sr I are provided, but are not corrected for NLTE effects. (Full table available at the CDS.)