\begin{table}%t2
\caption{\label{sat_lines}Selected \ion{Na}{ix} satellite lines excited by dielectronic recombination: data from the Cowan HFR code.} 
%\centerline
{\small
\begin{tabular}{l l l l l}
\hline\hline\noalign{\smallskip}
 Wavelength (\AA)\tablefootmark{a} &  Line label\tablefootmark{b} & Transition & $B_{\rm sat}$ (s$^{-1}$)\tablefootmark{c} & $E_{\rm sat}$ (Ry)  \\
 \hline\\[-3mm]
11.043 & $d15$ & $\rm 1s^2 3p~ ^2P_{1/2} {-} 1{\rm s} 2p 3p~ (^1P)~^2D_{3/2}$ & 3.33(13) & 73.5 \\
11.044 & $d13$ & $\rm 1s^2 3p~ ^2P_{3/2} {-} 1{\rm s} 2p 3p~ (^1P)~^2D_{5/2}$ & 5.77(13) & 73.5 \\
11.077\tablefootmark{d} & $s$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s} 2p^2~ (^3S)~^2P_{3/2}$ & 4.64(12) & 60.0 \\
11.078\tablefootmark{d} & $t$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^3S)~^2P_{1/2}$ & 2.90(12) & 60.0 \\
11.105 & $n$ &$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2S_{1/2}$ & 3.11(12) & 60.6 \\
11.108 & $m$ &$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2S_{1/2}$ & 8.19(12) & 60.6 \\
11.152\tablefootmark{d} & $q$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^1S)~^2P_{3/2}$ & 1.66(13) & 60.6 \\
11.155\tablefootmark{d} & $r$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~(^1S)~^2P_{1/2}$ & 9.61(12) & 60.6 \\
11.165 & $b$ &$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2P_{3/2}$ & 3.28(11) & 60.6 \\
11.168 & $d$ &$\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2P_{1/2}$ & 7.12(10) & 60.6 \\
11.168 & $a$ &$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2P_{3/2}$ & 2.13(12) & 60.6 \\
11.171 & $c$ &$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2P_{1/2}$ & 3.25(10) & 60.6 \\
11.188 & $k$ & $\rm 1s^2 2p~ ^2P_{1/2} {-} 1{\rm s} 2p^2~ ^2D_{3/2}$ & 2.31(13) & 60.6 \\
11.191 & $j$ &$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2D_{5/2}$ & 3.70(13) & 60.6 \\
11.192 & $l$ &$\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^2D_{3/2}$ & 1.90(12) & 60.6 \\
11.286 & $e$ & $\rm 1s^2 2p~ ^2P_{3/2} {-} 1{\rm s} 2p^2~ ^4P_{5/2}$ & 1.74(10) & 60.6 \\
11.298\tablefootmark{d} & $u$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s} 2p^2~ (^3S)^4P_{3/2}$ & 3.45(9) & 60.0 \\
11.300\tablefootmark{d} & $v$ & $\rm 1s^2 2s~ ^2S_{1/2} {-} 1{\rm s}2s2p~ (^3S)^4P_{1/2}$ & 6.64(8) & 60.0 \\
\hline
\end{tabular}}
\tablefoot{\tablefoottext{a}{Wavelengths from Cowan code + 0.001~\AA;} \tablefoottext{b}{Notation of \cite{gab72,bel79};} \tablefoottext{c}{Numbers in parentheses are powers of ten;} \tablefoottext{d}{Lines also formed by inner-shell excitation.}}
\end{table}