\begin{table}%t3
\caption {\label{tab:lines2} List of strongest \ion{Fe}{xvii}~lines in the 30--150~\AA\ range. 
}
%\centerline
 {\begin{tabular}{@{}llccrlllll@{}}
 \hline\hline    
 $i-j$ &  Transition  &  $Int$ &  $Int$ &   $\lambda_{\rm exp.}$(\AA) & $\lambda_{\rm CC}$(\AA)   &  $\lambda_{\rm NIST}$(\AA) &  $\lambda_{\rm MR-MP}$(\AA) & \\
  \hline
  &    & $1.0 \times 10^{11}$ & $1.0 \times 10^{19}$ &    & &  &  & \\ 
 \hline 
3--29 & 2s$^2$2p$^5$3s $^1$P$_{1}$--2p$^6$3s $^1$S$_{0}$ & 0.38 & 0.19 & 89.760 & 87.52&       87.319&        89.79 &   \\ 
5--56 & 2s$^2$2p$^5$3s $^3$P$_{1}$--2s$^2$2p$^5$4p $^1$S$_{0}$ & 0.15 & $7.2 \times 10^{-2}$ & 46.307 & 46.19& -- & --  &   \\ 
5--29 & 2s$^2$2p$^5$3s $^3$P$_{1}$--2p$^6$3s $^1$S$_{0}$ & 0.23 & 0.11 & 98.249 & 95.78&       95.317&        98.28 &   \\ 
3--47 & 2s$^2$2p$^5$3s $^1$P$_{1}$--2s$^2$2p$^5$4p $^3$P$_{0}$ & $8.4 \times 10^{-2}$ & $4.3 \times 10^{-2}$ & 46.300 & 46.12& -- & -  &   \\ 
8--53 & 2s$^2$2p$^5$3p $^3$D$_{3}$--2s$^2$2p$^5$4d $^3$F$_{4}$ & $6.4 \times 10^{-2}$ & 0.33 & 50.260 & 50.32&       50.280& --  &   \\ 
22--37 & 2s$^2$2p$^5$3d $^3$D$_{3}$--2p$^6$3d $^1$D$_{2}$ & 0.11 & 0.11 & 92.283 & 90.34& --&        92.35 &   \\ 
2--44 & 2s$^2$2p$^5$3s $^3$P$_{2}$--2s$^2$2p$^5$4p $^3$D$_{3}$ & $4.6 \times 10^{-2}$ & 0.16 & 46.400 & 46.64& -- & --  &   \\ 
33--119 & 2p$^6$3p $^1$P$_{1}$--2p$^6$4s $^1$S$_{0}$ & $5.4 \times  10^{-2}$ & $2.9 \times 10^{-2}$ & 57.710 & 57.79& -- & --  &   \\ 
33--135 & 2p$^6$3p $^1$P$_{1}$--2p$^6$4d $^1$D$_{2}$ & $4.6\times 10^{-2}$ & $4.0 \times 10^{-2}$ & 50.690 & 50.75& -- &--  &   \\ 
26--37 & 2s$^2$2p$^5$3d $^1$F$_{3}$--2p$^6$3d $^1$D$_{2}$ & $8.9 \times 10^{-2}$ & 
$8.9\times  10^{-2}$ & 100.640 & 98.53& -- &       100.71 &   \\ 
20--37 & 2s$^2$2p$^5$3d $^3$F$_{3}$--2p$^6$3d $^1$D$_{2}$ & $7.8 \times 10^{-2}$ & 
$7.9\times  10^{-2}$ & 90.401 & 88.51& -- &        90.47 &   \\ 
3--83 & 2s$^2$2p$^5$3s $^1$P$_{1}$--2s$^2$2p$^5$5p $^1$S$_{0}$ & 
$2.9 \times 10^{-2}$ & $7.1\times  10^{-3}$ &  --  & 33.73& -- & --  &   \\ 
14--70 & 2s$^2$2p$^5$3p $^1$D$_{2}$--2s$^2$2p$^5$4d $^1$F$_{3}$ & 
$4.2\times  10^{-2}$ & 0.14 &  --  & 50.46&-- & --  &   \\ 
13--69 & 2s$^2$2p$^5$3p $^3$P$_{1}$--2s$^2$2p$^5$4d $^3$D$_{2}$ & 
$4.1\times  10^{-2}$ & 0.11 &  --  & 50.44& -- & --  &   \\ 
27--56 & 2s$^2$2p$^5$3d $^1$P$_{1}$--2s$^2$2p$^5$4p $^1$S$_{0}$ & 
$5.5\times 10^{-2}$ & 
$2.6\times 10^{-2}$ & 68.510 & 68.66& -- & --  &   \\ 
7--55 & 2s$^2$2p$^5$3p $^3$D$_{2}$--2s$^2$2p$^5$4d $^3$F$_{3}$ & 
$3.9\times 10^{-2}$ & 0.18 & 49.870 & 49.93&       49.897& --  &   \\ 
19--36 & 2s$^2$2p$^5$3d $^3$F$_{4}$--2p$^6$3d $^3$D$_{3}$ & 
$7.1\times  10^{-2}$ & 0.25 &  --  & 91.29& -- &        93.20 &   \\ 
2--28 & 2s$^2$2p$^5$3s $^3$P$_{2}$--2p$^6$3s $^3$S$_{1}$ & $6.4 \times 10^{-2}$ & 0.21 &  --  & 90.52& -- &        92.50 &   \\ 
21--37 & 2s$^2$2p$^5$3d $^1$D$_{2}$--2p$^6$3d $^1$D$_{2}$ & $6.2 \times 0^{-2}$ & 
$6.2\times 10^{-2}$ & 91.550 & 89.60& -- &        91.62 &   \\ 
8--32 & 2s$^2$2p$^5$3p $^3$D$_{3}$--2p$^6$3p $^3$P$_{2}$ & 
$6.0\times 10^{-2}$ & 0.27 &  --  & 90.40& -- &        92.40 &   \\ 
6--52 & 2s$^2$2p$^5$3p $^3$S$_{1}$--2s$^2$2p$^5$4d $^3$P$_{1}$ & 
$3.1\times 10^{-2}$ & $6.6 \times 10^{-2}$ & 49.456 & 49.38&       49.443& --  &   \\ 
10--54 & 2s$^2$2p$^5$3p $^3$P$_{2}$--2s$^2$2p$^5$4d $^3$P$_{2}$ & $2.5\times  10^{-2}$ & $7.3\times 10^{-2}$ &  --  & 50.89& -- & --  &   \\ 
23--47 & 2s$^2$2p$^5$3d $^3$D$_{1}$--2s$^2$2p$^5$4p $^3$P$_{0}$ & $3.2\times  10^{-2}$ & $1.6\times  10^{-2}$ & 67.918 & 67.78& -- & --  &   \\ 
9--57 & 2s$^2$2p$^5$3p $^1$P$_{1}$--2s$^2$2p$^5$4d $^1$D$_{2}$ & $2.3 \times 10^{-2}$ & $8.4 \times 10^{-2}$ &  --  & 50.37&       49.805& --  &   \\ 
20--35 & 2s$^2$2p$^5$3d $^3$F$_{3}$--2p$^6$3d $^3$D$_{2}$ & $4.2 \times 10^{-2}$ & 0.11 &  --  & 92.03& -- &        93.91 &   \\ 8--38 & 2s$^2$2p$^5$3p $^3$D$_{3}$--2s$^2$2p$^5$4s $^3$P$_{2}$ & $2.1 \times 10^{-2}$ & 
$8.4\times  10^{-2}$ & 57.320 & 57.40&       57.331& --  &   \\ 
14--42 & 2s$^2$2p$^5$3p $^1$D$_{2}$--2s$^2$2p$^5$4s $^3$P$_{1}$ & 
$1.9\times 10^{-2}$ & $3.7\times 10^{-2}$ & 57.536 & 57.68&       57.646& --  &   \\ 
11--59 & 2s$^2$2p$^5$3p $^3$P$_{0}$--2s$^2$2p$^5$4d $^3$D$_{1}$ & 
$1.6\times 10^{-2}$ & 
$1.7\times 10^{-2}$ & 51.247 & 51.29&       51.236& --  &   \\ 
25--37 & 2s$^2$2p$^5$3d $^3$D$_{2}$--2p$^6$3d $^1$D$_{2}$ & 
$3.1\times 10^{-2}$ & 
$3.1\times 10^{-2}$ & 100.211 & 98.06& -- &       100.29 &   \\ 
24--37 & 2s$^2$2p$^5$3d $^3$F$_{2}$--2p$^6$3d $^1$D$_{2}$ & 
$3.0\times 10^{-2}$ & 
$3.0\times 10^{-2}$ & 99.553 & 97.45& -- &        99.63 &   \\ 
9--59 & 2s$^2$2p$^5$3p $^1$P$_{1}$--2s$^2$2p$^5$4d $^3$D$_{1}$ & $1.5 \times 10^{-2}$ & 
$1.6\times  10^{-2}$ & 49.750 & 49.75&       49.748& --  &   \\ 
15--71 & 2s$^2$2p$^5$3p $^1$S$_{0}$--2s$^2$2p$^5$4d $^1$P$_{1}$ & $1.5\times 10^{-2}$ &
 $1.7\times 10^{-2}$ & 52.780 & 53.25&       52.754& --  &   \\ 
19--62 & 2s$^2$2p$^5$3d $^3$F$_{4}$--2s$^2$2p$^5$4f $^3$G$_{5}$ & $1.4\times  10^{-2}$ & 0.69 & 58.760 & 58.93&       58.783& --  &   \\ 
7--57 & 2s$^2$2p$^5$3p $^3$D$_{2}$--2s$^2$2p$^5$4d $^1$D$_{2}$ & $1.1\times  10^{-2}$ & 
$4.0\times  10^{-2}$ &  --  & 49.80&       49.261& --  &   \\ 
21--34 & 2s$^2$2p$^5$3d $^1$D$_{2}$--2p$^6$3d $^3$D$_{1}$ & $1.9\times  10^{-2}$ & $4.7\times  10^{-2}$ &  --  & 93.34& -- &        95.25 &   \\ 
25--74 & 2s$^2$2p$^5$3d $^3$D$_{2}$--2s$^2$2p$^5$4f $^3$D$_{3}$ & $1.2 \times 10^{-2}$ & 0.25 & 58.980 & 59.23&       59.240& --  &   \\ 
17--63 & 2s$^2$2p$^5$3d $^3$P$_{1}$--2s$^2$2p$^5$4f $^3$D$_{2}$ & $1.2\times  10^{-2}$ & 0.11 &  --  & 58.33&       58.268& -- &   \\ 
26--73 & 2s$^2$2p$^5$3d $^1$F$_{3}$--2s$^2$2p$^5$4f $^3$G$_{4}$ & $1.2 \times 10^{-2}$ & 0.30 & 59.258 & 59.43& -- & --  &   \\ 
9--39 & 2s$^2$2p$^5$3p $^1$P$_{1}$--2s$^2$2p$^5$4s $^1$P$_{1}$ & $1.1 \times 10^{-2}$ & $2.1 \times 10^{-2}$ & 57.388 & 57.53&       57.407& --  &   \\ 
20--61 & 2s$^2$2p$^5$3d $^3$F$_{3}$--2s$^2$2p$^5$4f $^1$G$_{4}$ & $1.1\times  10^{-2}$ & 0.41 & 58.980 & 59.15&       59.278& --  &   \\ 
7--39 & 2s$^2$2p$^5$3p $^3$D$_{2}$--2s$^2$2p$^5$4s $^1$P$_{1}$ & $1.1 \times 10^{-2}$ & 
$2.0\times 10^{-2}$ & 56.668 & 56.79&       56.686& --  &   \\ 
18--37 & 2s$^2$2p$^5$3d $^3$P$_{2}$--2p$^6$3d $^1$D$_{2}$ & $1.6 \times 10^{-2}$ & $1.6 \times 10^{-2}$ & 89.874 & 87.92& -- &        89.95 &   \\ 
10-39 & 2s$^2$2p$^5$3p $^3$P$_{2}$--2s$^2$2p$^5$4s $^1$P$_{1}$ & $1.0 \times 10^{-2}$ & 
$1.9\times  10^{-2}$ & 57.874 & 58.01&       57.893& --  &   \\ 
27--37 & 2s$^2$2p$^5$3d $^1$P$_{1}$--2p$^6$3d $^1$D$_{2}$ & $1.8 \times 10^{-2}$ & $1.8\times 10^{-2}$ & 106.585 & 104.77& -- &       106.66 &   \\ 
7--31 & 2s$^2$2p$^5$3p $^3$D$_{2}$--2p$^6$3p $^3$P$_{1}$ &
 $1.5\times  10^{-2}$ & 
$6.5\times  10^{-2}$ & 92.793 & 90.86&       92.832&        92.89 &   \\ 
18--64 & 2s$^2$2p$^5$3d $^3$P$_{2}$--2s$^2$2p$^5$4f $^3$F$_{3}$ &$ 8.7 \times 10^{-3}$ & 0.27 & 58.621 & 58.76& -- & --  &   \\ 
24--72 & 2s$^2$2p$^5$3d $^3$F$_{2}$--2s$^2$2p$^5$4f $^3$G$_{3}$ & $8.2\times 10^{-3}$ & 0.22 & 58.751 & 59.07&       59.010& --  &   \\ 
22--67 & 2s$^2$2p$^5$3d $^3$D$_{3}$--2s$^2$2p$^5$4f $^3$F$_{4}$ & $7.9 \times 10^{-3}$ & 0.40 & 59.590 & 59.79&       59.607& --  &   \\ 
21--66 & 2s$^2$2p$^5$3d $^1$D$_{2}$--2s$^2$2p$^5$4f $^1$F$_{3}$ & $7.4 \times 10^{-3}$ & 0.25 & 59.260 & 59.48&       59.337& --  &   \\ 
 \hline                                   %inserts single line
\end{tabular}}
\par
\smallskip
Notes:  Lines are ordered by decreasing intensity. 
The first column indicates the level indices as given 
in \cite{loch_etal:06}.
The second column provides the transition description.  
The  relative intensities  (photons) $Int$ 
were calculated at electron densities of 10$^{11}$ and  10$^{19}$~cm$^{-3}$, typical 
of solar flares and laboratory spectra.
 $\lambda_{\rm exp.}$ are our experimental wavelengths.
$\lambda_{\rm CC}$  are the wavelengths obtained from the  scattering target energies
 \citep{loch_etal:06}, while  $\lambda_{\rm NIST}$ 
are those from NIST~v.3 and  $\lambda_{\rm MR-MP}$ are those obtained from the MR-MP calculations. 
%\vspace*{4mm}
\end{table}