\begin{table}%T4
\caption{\label{fr_ne}Measured line counts for Ne~{\sc ix} resonance~($r$) and forbidden ($f$)~lines and Ne~{\sc ix} luminosities $L_{\rm Ne~\mathsc{ix}}$ from summed~($r+i+f$)~line fluxes.}
%\begin{center}
{{\scriptsize
\begin{tabular}{p{.8cm}p{.7cm}ccc}
\hline\hline
 star & Instr.& $r$ & $f$ &log($L_{\rm Ne~\mathsc{ix}}$)$^a$\\
 \hline
         47~Cas&  RGS2&  452.00~$\pm$~38.77&  278.85~$\pm$~28.22&    28.64~$\pm$~0.04\\
         AB~Dor&  RGS2&  1614.6~$\pm$~57.63&  1030.0~$\pm$~50.39&    28.45~$\pm$~0.01\\
 &   MEG&  524.16~$\pm$~26.51&  290.84~$\pm$~18.73&    28.34~$\pm$~0.02\\
 &   HEG&  110.99~$\pm$~10.98&  77.682~$\pm$~9.189&    28.33~$\pm$~0.05\\
         AD~Leo&  RGS2&  553.77~$\pm$~37.81&  400.75~$\pm$~29.26&    27.22~$\pm$~0.03\\
 &  LETG&  276.32~$\pm$~19.20&  165.42~$\pm$~16.04&    27.16~$\pm$~0.04\\
           Algol&  LETG&  631.23~$\pm$~36.62&  347.91~$\pm$~31.94&    28.83~$\pm$~0.04\\
 &   MEG&  283.27~$\pm$~23.00&  194.68~$\pm$~18.40&    28.65~$\pm$~0.04\\
 &   HEG&  79.109~$\pm$~9.973&  57.690~$\pm$~8.389&    28.79~$\pm$~0.06\\
         AR~Lac&  RGS2&  488.50~$\pm$~42.06&  364.31~$\pm$~33.39&    29.12~$\pm$~0.04\\
 &   MEG&  152.66~$\pm$~14.84&  136.82~$\pm$~13.30&    29.00~$\pm$~0.05\\
 &   HEG&  39.833~$\pm$~6.650&  15.984~$\pm$~4.306&    28.93~$\pm$~0.10\\
         AT~Mic&  RGS2&  632.39~$\pm$~34.03&  387.00~$\pm$~28.22&    28.03~$\pm$~0.02\\
         AU~Mic&  RGS2&  1156.9~$\pm$~45.71&  812.28~$\pm$~41.49&    27.97~$\pm$~0.02\\
 &   MEG&  319.98~$\pm$~19.79&  212.47~$\pm$~15.78&    27.74~$\pm$~0.03\\
 &   HEG&  87.094~$\pm$~9.526&  52.332~$\pm$~7.293&    27.80~$\pm$~0.06\\
    $\beta$~Cet&  LETG&  679.75~$\pm$~41.78&  465.82~$\pm$~35.45&    28.78~$\pm$~0.03\\
 &   MEG&  363.20~$\pm$~23.78&  211.92~$\pm$~17.14&    28.58~$\pm$~0.03\\
 &   HEG&  82.103~$\pm$~9.361&  64.720~$\pm$~8.301&    28.61~$\pm$~0.06\\
         Capella&  LETG&  3960.8~$\pm$~79.78&  2312.8~$\pm$~66.94&    28.58~$\pm$~0.01\\
 &   MEG&  2512.9~$\pm$~60.13&  1373.2~$\pm$~42.87&    28.43~$\pm$~0.01\\
 &   HEG&  616.43~$\pm$~25.70&  373.48~$\pm$~20.09&    28.46~$\pm$~0.02\\
         EK~Dra&  RGS2&  172.87~$\pm$~20.22&  139.63~$\pm$~18.39&    28.47~$\pm$~0.05\\
 $\epsilon$~Eri&  RGS2&  213.28~$\pm$~19.03&  125.74~$\pm$~16.75&    26.87~$\pm$~0.04\\
 &  LETG&  564.02~$\pm$~27.20&  347.98~$\pm$~22.35&    26.82~$\pm$~0.02\\
         EQ~Peg&  RGS2&  209.59~$\pm$~23.72&  154.66~$\pm$~18.08&    27.41~$\pm$~0.05\\
         EV~Lac&  RGS2&  376.34~$\pm$~31.23&  253.93~$\pm$~24.17&    27.14~$\pm$~0.04\\
 &   MEG&  454.53~$\pm$~23.74&  222.32~$\pm$~16.34&    27.02~$\pm$~0.03\\
 &   HEG&  115.34~$\pm$~11.01&  68.823~$\pm$~8.547&    27.08~$\pm$~0.05\\
        HR~1099&  RGS2&  762.77~$\pm$~44.32&  409.12~$\pm$~36.44&    29.03~$\pm$~0.03\\
 &  LETG&  1231.7~$\pm$~45.61&  727.60~$\pm$~39.44&    29.09~$\pm$~0.02\\
 &   MEG&  1690.5~$\pm$~50.43&  834.17~$\pm$~34.81&    29.13~$\pm$~0.01\\
 &   HEG&  477.47~$\pm$~22.85&  228.75~$\pm$~16.25&    29.21~$\pm$~0.02\\
   $\kappa$~Cet&  RGS2&  251.60~$\pm$~23.27&  193.82~$\pm$~21.53&    27.40~$\pm$~0.04\\
  $\lambda$~And&  RGS2&  532.86~$\pm$~39.36&  335.00~$\pm$~33.78&    28.71~$\pm$~0.03\\
 &   MEG&  506.89~$\pm$~26.09&  219.34~$\pm$~17.80&    28.55~$\pm$~0.03\\
 &   HEG&  54.933~$\pm$~7.704&  35.636~$\pm$~6.216&    28.28~$\pm$~0.08\\
    $\pi^1$~UMa&  RGS2&  158.38~$\pm$~19.24&  105.83~$\pm$~15.87&    27.46~$\pm$~0.06\\
         Procyon&  LETG&  66.930~$\pm$~10.46&  35.030~$\pm$~8.468&    25.83~$\pm$~0.10\\
   $\sigma$~CrB&  RGS2&  693.59~$\pm$~48.82&  344.81~$\pm$~37.72&    28.86~$\pm$~0.03\\
         UX~Ari&  RGS2&  671.37~$\pm$~40.05&  456.80~$\pm$~33.42&    29.42~$\pm$~0.02\\
 &  LETG&  564.02~$\pm$~27.20&  347.98~$\pm$~22.35&    29.19~$\pm$~0.02\\
 &   MEG&  409.21~$\pm$~23.32&  237.38~$\pm$~17.32&    29.33~$\pm$~0.03\\
 &   HEG&  48.597~$\pm$~7.493&  18.571~$\pm$~4.596&    28.95~$\pm$~0.10\\
         VY~Ari&  RGS2&  481.21~$\pm$~33.86&  306.33~$\pm$~28.95&    29.11~$\pm$~0.03\\
         YY~Gem&  LETG&  240.53~$\pm$~18.54&  137.45~$\pm$~15.34&    28.06~$\pm$~0.05\\
         YZ~CMi&  RGS2&  195.54~$\pm$~22.57&  101.04~$\pm$~15.84&    27.01~$\pm$~0.06\\
\hline
\end{tabular}}}
{
$^a$ In erg/s.}
%\end{center}
\par
\end{table}