\begin{table}%t3
\caption{\label{tabfit}$A$(N) of \ion{N}{i} from line fitting using 1D models with SYNTHE.}
\small%\centerline
 {
\begin{tabular}{cccccc}
\hline\hline
Observed & $\lambda$&\multicolumn{3}{c}{$A$(N)$_{\rm LTE}$} & $A$(N)$_{\rm NLTE}$ \\
spectrum &  (nm)      & HM & ATLAS9 & \mD\ & \mD\ \\
\hline
KF &  746.8 & 7.861 & 7.824 & 7.809 & 7.750 \\
NF &  746.8 & 7.874 & 7.837 & 7.827 & 7.768 \\
NI &  746.8 & 7.890 & 7.834 & 7.823 & 7.785 \\
DI &  746.8 & 7.908 & 7.849 & 7.840 & 7.802 \\
\hline
KF &  821.6 & 7.847 & 7.811 & 7.805 & 7.730 \\
NF &  821.6 & 7.918 & 7.870 & 7.867 & 7.792 \\
NI &  821.6 & 7.944 & 7.879 & 7.873 & 7.821 \\
DI &  821.6 & 7.808 & 7.752 & 7.746 & 7.694 \\
\hline
KF &  868.3 & 7.910 & 7.889 & 7.857 & 7.783 \\
NF &  868.3 & 7.906 & 7.877 & 7.857 & 7.783 \\
NI &  868.3 & 7.933 & 7.878 & 7.875 & 7.831 \\
DI &  868.3 & 7.932 & 7.886 & 7.882 & 7.838 \\
\hline
\end{tabular}}
\medskip
Notes: Col.~(1) is the observed spectrum identification, KF: Kurucz Flux, NF: Neckel Flux,
NI: Neckel Intensity, and DI: Delbouille Intensity; Col.~(2) is the wavelength; Cols.~(3)$-$(5) the $A$(N)$_{\rm LTE}$ from line fitting with HM, ATLAS9, and \mD~model; Col.~(6) is the $A$(N)$_{\rm NLTE}$ for the \mD~model, obtained by adding the NLTE-correction computed with $S_{\rm H}=1/3$ to the abundances given in~Col.~(5).
\end{table}