All Tables

Table 1: Ranges and steps of model parameters.
Table 2: Adopted $\log gf$ values of important lines in the VLT/UVES spectrum. This line list do not included the weaker lines which these lines are blended with. The best fit abundance computed in LTE, [X/H], is also given for each feature.
Table 3: Same as Table 2 but for the important lines in the Keck I/HIRES spectrum.
Table 4: Chemical abundances of the secondary star in Nova Scorpii 1994.