\begin{table}%t7
%\centering
\par
\caption{Summary of the line identifications for \ion{Fe}{x} 
(see the Appendix for details). 
The columns indicate: 
1) the  indexes corresponding to Table~\ref{tab:levels};
2) the relative intensity (at 10$^8$~\cmt), scaled to the brightest line;
3) the  wavelengths calculated from our best energies $E_{\rm best}$;
4) observed solar wavelengths~$\lambda_{\rm solar}$ 
  (unless specified otherwise values are from \citealt{behring_etal:76}); 
 some blends are indicated (bl~=~blend; \mbox{bl-mr~=~blend} in medium-resolution spectra;
bl-w~=~blend with a weak line); 
lines with no or a tentative identification have a question mark; 5 and~6) previous identifications consistent or not with ours 
(with  observed  wavelengths in~\AA; note that 
 observed and calculated wavelengths in the cited literature
can differ from the values reported here).
Legenda:
B~=~\cite{bromage_etal:77};
BR~=~\cite{brooks_etal:99};
BD~=~\cite{bhatia_doschek:95};
%D~=~\cite{delzanna_thesis99};
E42~=~\cite{edlen:42};
E~=~\cite{edlen:69};
ES~=~\cite{edlen_smitt:78};
FG~=~\cite{fawcett_gabriel:66};
F~=~\cite{fawcett:71};
FE~=~\cite{feldman_etal:97};
G~=~\cite{gabriel_etal:66};
J~=~\cite{jupen_etal:93};
JE~=~\cite{jefferies_etal:71} (wavelengths in air);
M~=~\cite{mason_nussbaumer:77};
MH~=~\cite{malinovsky_heroux:73};
MC~=~\cite{magnant-crifo:73};
S~=~\cite{smitt:77};
SBT~=~\cite{sandlin_etal:77};
ST~=~\cite{sandlin_tousey:79};
TN~=~\cite{thomas_neupert:94}.
\label{tab:id}}
\begin{tabular}[c]{@{}cclllll@{}}
\hline\hline\noalign{\smallskip}
 $i{-}j$    & Rel. $I$  & $\lambda$ (\AA) & $\lambda_{\rm solar}$ (\AA) & Same ID & Diff. ID & \\
\hline\noalign{\smallskip}
\par
1--31 & $1.8 \times 10^{-3}$  & 170.575~$\pm$~0.001 & ? 170.58 (FG) & FG,~B,~BD  &    \\
\par
1--30 &  1.0 & 174.531~$\pm$~0.002 & 174.531~$\pm$~0.002  (bl-w \ion{Fe}{ix}) & G,~FG,~MH,~B,~BD &  \\ 
\par
2--31 & $4.1 \times 10^{-2}$ &  175.263~$\pm$~0.002 & 175.263~$\pm$~0.004 (bl-mr) & G,~FG,~MH,~B,~BD & \\ 
1--29 & $1.8  \times 10^{-2}$ & 175.475~$\pm$~0.006 & 175.475~$\pm$~0.01 (bl-mr, bl-w \ion{Fe}{ix}) & FG, MH, B, BD & \\ 
\par
1--28 & 0.55 & 177.240~$\pm$~0.002 & 177.239~$\pm$~0.002 & G,~FG,~MH,~B,~BD &  & \\ 
\par
2--29 & $5.6 \times  10^{-2}$ &  180.441~$\pm$~0.007 & ? 180.401~$\pm$~0.002 (bl \ion{Fe}{xi}) & FG,~B,~BD & & \\ 
\par
2--28 & $1.5 \times  10^{-2}$ & 182.307~$\pm$~0.002  & 182.308~$\pm$~0.01 (bl-mr \ion{Fe}{xi} 182.167) & FG,~MH,~B,~BD & &  \\
\par
1--27 & 0.22 & 184.537~$\pm$~0.002 & 184.536~$\pm$~0.002 & FG,~MH,~B,~BD & & \\ 
\par
2--27 & $6.5 \times  10^{-2}$ &  190.037~$\pm$~0.002 & 190.038~$\pm$~0.002 (bl-mr)  & FG,~B,~BD & MH & \\ 
\par
1--26 &  $8.7  \times 10^{-3}$ & 193.715~$\pm$~0.019  & ? 193.715~$\pm$~0.01  & J(193.715) & BD(188.927) & \\
\par
%level not id.
1--25 &  $5.7  \times 10^{-3}$ & 195.316~$\pm$~0.19 & ? 195.399 (B) & B &  & \\
%level not id.
2--25 &  $2.2 \times  10^{-3}$ & 201.487~$\pm$~0.20  & ? 201.556 (B) & B &  & \\
\par
1--23 & $1.4 \times  10^{-2}$ & 207.449~$\pm$~0.022  & ? 207.449~$\pm$~0.004 & J(207.444) & B?(209.776),~BD(204.145) &  \\ 
\par
1--22 & $2.3 \times  10^{-2}$ &  220.247~$\pm$~0.024  & ? 220.247~$\pm$~0.01 (bl) & J & B?(220.882),~BD & \\ 
%\footnote{\cite{jupen_etal:93} does not provide a laboratory wavelength and \cite{bromage_etal:77} gave a tentative ID.}
\par
1--19 & $2.7 \times  10^{-2}$ & 225.856~$\pm$~0.253  & ? 225.856~$\pm$~0.004 (bl) & & J(225.16) BD(222.96) & \\ 
\par
%??
1--17 & $2.5 \times  10^{-2}$ &  227.208~$\pm$~0.258 & ? 227.208~$\pm$~0.01  (bl) &  & B(226.31),~BD(226.32) & \\ 
\par
%1-18 &  1.5 10$^{-2}$ &  226.840~$\pm$~0.003 & ?                  & & & \\ 
\par
1--14 & $9.3 \times  10^{-3}$  & 230.667~$\pm$~0.27   & ? 230.127~$\pm$~0.01 &        & B(229.99),~J(229.969) & \\
\par
%level 15 not id.
1--15 &  $1.1  \times 10^{-2}$ & 230.900~$\pm$~0.264  & ?   & & B(230.089),~BD  & \\ 
\par
%1-12 very weak line -
%1-16 very weak line -
\par
1--11 & $1.7 \times  10^{-2}$ & 234.599~$\pm$~0.27  & ? 234.356~$\pm$~0.004 (bl \ion{He}{ii}) & S,~B,~J(234.353),~BD & & \\
\par
%level 13 not id.
1--13 & $1.6 \times  10^{-2}$ & 236.494~$\pm$~0.279  & ? 236.494~$\pm$~0.01  &     & J(233.53 bl \ion{O}{v}),~BD(231.52) &  \\
\par
%level not id. - very weak line.
%2-15 & 6.1 10$^{-3}$  &  & & ? 238.72 (B) & B,BD   &\\
\par
%level not id.
%2-13 & 5.2 10$^{-3}$  & 245.701~$\pm$~0.30  & ? &  & B(240.243)& \\
\par
1--6 &  $1.3  \times 10^{-2}$ & 256.398~$\pm$~0.033  & ? 256.38~$\pm$~0.02 (bl \ion{Si}{x}) & S,~B,~J(256.405 bl),~BD & & \\ 
1--5 &   0.14         & 257.263~$\pm$~0.003  & 257.262~$\pm$~0.002 (bl-mr)  &  & & \\ 
1--4 &  $3.2  \times 10^{-2}$ & 257.259~$\pm$~0.003  &   ''  & S,~B,~J(257.257),~BD  & & \\ 
\par
5--35  & $2.9  \times 10^{-3}$ & 327.314~$\pm$~0.54  & ? 327.8 (BR)   & & S(324.726), BD & \\
\par
%ok
18--43 & $2.0  \times10^{-2}$ & 337.235~$\pm$~0.04   & 337.238 (TN)        &  & BD(296.194) & \\ 
\par
1--3 & $8.2 \times  10^{-2}$ &  345.738~$\pm$~0.006  & 345.739~$\pm$~0.004 & F,~BD & & \\ 
\par
%ok
21--43 & $7.9  \times 10^{-3}$ & 349.302~$\pm$~0.043 & ? bl \ion{Mg}{vi},\ion{Fe}{xi} 349.162 (TN)     &  &BD(288.063)& \\ 
\par
2--3 & $3.6 \times  10^{-2}$ &  365.560~$\pm$~0.008  & 365.54~$\pm$~0.02 (bl \ion{Ne}{v}) & F(365.57) & & \\ 
\par
5--24 & $6.8  \times 10^{-3}$ & 1028.02~$\pm$~0.1 &  1028.02 (FE)  & BD, FE & & \\ 
4--24 & $1.8 \times  10^{-3}$ & 1028.08~$\pm$~0.1  &   ''  & BD & & \\ 
8--24 & $7.6 \times  10^{-3}$ & 1463.49~$\pm$~0.2 & 1463.49~$\pm$~0.01 (SBT)  & ?M,~S,~ES,~BD  & & \\ 
\par
%??????? check
10--24& $1.7 \times  10^{-5}$ & 1582.35~$\pm$~0.4 & ?   &  & S,ES(1582.56),~?BD & \\
\par
5--21 & $5.8  \times 10^{-3}$ & 1603.21~$\pm$~0.3 & 1603.21~$\pm$~0.01 (ST) & M,~S,~ES,~BD & & \\ 
4--21 & $2.8  \times 10^{-3}$ & 1603.35~$\pm$~0.3 & 1603.35~$\pm$~0.04 (ST) &  & & \\ 
\par
5--20 & $1.9  \times 10^{-3}$ & 1611.71~$\pm$~0.3 & 1611.70~$\pm$~0.05 (SBT) & S,~ES,~BD & & \\ 
\par
5--18 & $1.4  \times 10^{-2}$ & 1918.24~$\pm$~0.4 & 1918.25  (SBT,ST)   & M,~S,~ES,~BD& & \\ 
4--18 & $2.4  \times 10^{-3}$ & 1918.45~$\pm$~0.4  &  ''    & S, ES, BD & & \\ 
\par
5--10 & $1.7  \times 10^{-2}$ & 2934.5~$\pm$~1.3 &  ?   & BD(2933.756) & E(3124) & \\ 
\par
%???
8--20 & $2.2 \times 10^{-2}$ & 3021.0~$\pm$~0.9 & ? 3020.1 (MC)  & S,~ES,~BD & & \\ 
5--8 &  $6.4 \times 10^{-2}$ & 3454.9~$\pm$~1.2 & 3454.2 (JE) &  M,~S,~ES,~BD & E(3800.8) &  \\ 
\par
10--21 & $5.3  \times 10^{-3}$ & 3533.8~$\pm$~1.9 &  3533.6 (JE) & M,~S,~ES & E(3338.5) & \\ 
10--20 & $1.8 \times  10^{-3}$  & 3575.4~$\pm$~1.9  & 3577.1 (JE) & S,~ES & & \\ 
\par
8--18 &  $5.6 \times  10^{-3}$ & 4312.8~$\pm$~1.9  &  4311.8 (JE) & M,~S,~ES & & \\ 
\par
10--18 & $3.9  \times  10^{-3}$ & 5538.9~$\pm$~4.6 & 5539.1 (JE) & S,~ES  & & \\ 
\par
1--2 &  0.88 &  6376.3~$\pm$~0.4  & 6374.6 (JE)  &  E42, M,~S,~ES,~BD & & \\ 
\hline
\end{tabular}
\end{table}