\begin{table}%t1
\caption{Photometric results for NK~1 (top) and SK~1 (bottom). 
The upper energy level of the transition is given in the third~column. The $x$ and $y$~peak position offsets are relative to the 1--0~S(1)~peak position.}
\label{nk1sk1_fluxes}
\small%%\centering

\par
\begin{tabular}{l@{~~~}r@{~~~}r@{}rrrr}
\hline \hline
\noalign{\smallskip}
{NK~1} & {$\lambda$} & {$T$~~~} &{total~flux~$^{\ast}$} &{peak~flux~$^{\dagger}$} &{$x$~offset} &{$y$~offset}\\
{line}&{($\mu$m)} &{(K)~} &{} &{} &{(arcsec)} &{(arcsec)}\\
& & & &{} & &\\
\hline   
{Fe\small{[II]}} &{1.644} &{11300} &{18.8} &{10.9} &{--0.05} &{0.16} \\
{(1,0)~S(7)} &{1.747} &{12817} &{16.1} &{10.5} &{0.18} &{0.12} \\
{(1,0)~S(6)} &{1.788} &{11522} &{15.8} &{7.4}  &{0.08} &{--0.01}\\
{(1,0)~S(5)} &{1.835} &{10341} &{40.5} &{32.2} &{0.06} &{0.10} \\
{(1,0)~S(4)} &{1.891} &{9286}  &{29.3} &{17.4} &{0.10} &{0.02} \\
{(1,0)~S(3)} &{1.957} &{8365} &{137.0} &{65.2} &{0.06} &{0.06} \\
{(1,0)~S(2)} &{2.033} &{7584}  &{40.7} &{19.2} &{0.02} &{0.03} \\
{(2,1)~S(3)} &{2.073} &{13890} &{12.9} &{8.1}  &{0.12} &{0.05} \\
{(1,0)~S(1)} &{2.121} &{6956} &{122.7} &{48.7} &{0.00} &{0.00} \\
{(2,1)~S(2)} &{2.154} &{13150} &{5.2}  &{3.9}  &{0.06} &{0.10} \\
{(1,0)~S(0)} &{2.223} &{6471}  &{30.7} &{15.2} &{--0.04}&{0.09} \\
{(2,1)~S(1)} &{2.247} &{12550} &{12.5} &{7.3}  &{0.10} &{0.08} \\
{(1,0)~Q(1)} &{2.406} &{6149}  &{112.3}&{47.4} &{--0.07}&{0.07} \\
{(1,0)~Q(2)} &{2.413} &{6471}  &{30.9} &{16.3} &{--0.04}&{0.05} \\
{(1,0)~Q(3)} &{2.423} &{6956}  &{109.6}&{45.4} &{--0.07}&{0.02} \\
{(1,0)~Q(4)} &{2.437} &{7584}  &{31.8} &{17.2} &{--0.05}&{0.07} \\
{(1,0)~Q(5)} &{2.454} &{8365}  &{43.0} &{20.8} &{0.11} &{--0.05}\\
\hline
\end{tabular}\\
\par
\begin{tabular}{l@{~~~}r@{~~~}r@{}rrrr}
\hline \hline
\noalign{\smallskip}
{SK~1} & {$\lambda$} &{$T$~~~} &{total~flux~$^{\ast\ast}$} &{peak~flux~$^{\dagger}$} &{$x$~offset} &{$y$~offset}\\
{line}&{($\mu$m)} &{(K)~} &{} &{} &{(arcsec)} &{(arcsec)}\\
\hline 
{Fe\small{[II]}} &{1.644} &{11300} &{10.1} &{18.0} &{0.03} &{--0.19} \\
{(1,0)~S(9)}  &{1.687}   &{15722} &{3.1}  &{5.6}  &{0.27} &{--0.31} \\
{(1,0)~S(8)}  &{1.714}   &{14221} &{2.9}  &{7.6}  &{0.14} &{--0.21} \\
{(1,0)~S(7)}  &{1.747}   &{12817} &{23.4} &{23.4} &{0.06} &{--0.08} \\
{(1,0)~S(6)}  &{1.788}   &{11522} &{13.2} &{14.3} &{0.10} &{--0.04} \\
{(1,0)~S(5)}  &{1.835}   &{10341} &{38.7} &{39.1} &{0.03} &{--0.06} \\
{(1,0)~S(4)}  &{1.891}   &{9286}  &{33.7} &{21.0} &{0.10} &{--0.07} \\
{(1,0)~S(3)}  &{1.957}   &{8365}  &{145.9}&{101.2}&{0.05} &{--0.01} \\
{(1,0)~S(2)}  &{2.033}   &{7584}  &{43.0} &{32.1} &{0.02} &{--0.01} \\
{(2,1)~S(3)}  &{2.073}   &{13890} &{22.2} &{21.8} &{0.05} &{--0.09} \\
{(1,0)~S(1)}  &{2.121}   &{6956}  &{150.2}&{109.9}&{0.00} &{0.00}  \\
{(2,1)~S(2)}  &{2.154}   &{13150} &{6.4}  &{8.2}  &{0.11} &{--0.07} \\
{(3,2)~S(3)}  &{2.201}   &{19086} &{5.2}  &{6.5}  &{0.05} &{--0.14} \\
{(1,0)~S(0)}  &{2.223}   &{6471}  &{30.3} &{22.9} &{0.01} &{--0.02} \\
{(2,1)~S(1)}  &{2.247}   &{12550} &{23.3} &{19.8} &{0.06} &{--0.06} \\
{(2,1)~S(0)}  &{2.355}   &{12095} &{4.2}  &{6.3}  &{0.00} &{--0.15} \\
{(1,0)~Q(1)}  &{2.406}   &{6149}  &{134.8}&{87.7} &{0.01} &{0.00}  \\
{(1,0)~Q(2)}  &{2.413}   &{6471}  &{42.4} &{30.6} &{0.02} &{--0.02} \\
{(1,0)~Q(3)}  &{2.423}   &{6956}  &{137.9}&{96.2} &{0.01} &{--0.02} \\
{(1,0)~Q(4)}  &{2.437}   &{7584}  &{42.5} &{34.1} &{0.02} &{--0.03} \\
{(1,0)~Q(5)}  &{2.454}   &{8365}  &{85.3} &{64.9} &{0.02} &{--0.01} \\
{(1,0)~Q(6)}  &{2.475}   &{9286}  &{29.1} &{23.7} &{0.07} &{0.00}  \\
\hline
\end{tabular}
\begin{flushleft}
$\ast$ Units of $10^{-18}$ W~m$^{-2}$. The 1$\sigma$~flux measurement uncertainty is 2.6~$\times$ 
10$^{-18}$~W~m$^{-2}$ and 5.2~$\times$ 10$^{-18}$~W~m$^{-2}$ beyond 2.4~$\mu$m. This (standard deviation) value was derived from a~large sample of flux measurements within apertures placed on sky regions and at various wavelengths.  \\
$\ast\ast$ Units of $10^{-18}$~W~m$^{-2}$. The 1$\sigma$~flux measurement uncertainty is 3.3~$\times$ 10$^{-18}$~W~m$^{-2}$ and 6.6~$\times$ 10$^{-18}$~W~m$^{-2}$ beyond 2.4~$\mu$m.\\
$\dagger$ Units of $10^{-18}$~W~m$^{-2}$~arcsec$^{-2}$. The 1$\sigma$~noise level is 
1.0~$\times$ 10$^{-18}$~W~m$^{-2}$~arcsec$^{-2}$.
\end{flushleft}
\end{table}