\begin{table}%t3
%%%%\centering
\par
\caption{WR~25 emission-line wavelengths and fluxes as observed with
         {\it XMM} {\sc rgs1~+~2} and {\sc epic-mos}. Values within
         parentheses are the 1~$\sigma$ uncertainties. }
\begin{tabular}{rlrlrcll}
\hline \hline 
\multicolumn{2}{c}{{\sc rgs1}~+~{\sc rgs2}}&\multicolumn{2}{c}{\sc epic-mos} & \multicolumn{4}{c}{identification$^a$}  \\
\hline
$\lambda$(\AA) & flux$^b$ & $\lambda$(\AA) & flux$^b$  & $\lambda$(\AA) & \multicolumn{1}{c}{$E$ (keV)} & ion & type$^c$  \\
\hline
              &           &                &           &                &         &                                 \\[-2mm]
  ---         & ---       &  1.86          & 0.05      &  1.87~~       & 6.63~~ & \Fexxv   & K$\alpha$   \\
  ---         & ---       &  3.98          & 0.04      &  3.97~~       & 3.12~~ & \Sxvi    & Ly$\beta$   \\
              &           &                &           &  3.97~~       & 3.12~~ & \Arxvii  & He4         \\
  ---         & ---       &  5.08          & 0.15(.03) &  5.04~~       & 2.45~~ & \Sxv     & He4         \\
  ---         & ---       &  5.7           & ---       &  5.64~~       & 2.20~~ & \Sixiii  & He3         \\
  ---         & ---       &  6.2           & 0.14(.03) &  6.20~~       & 2.00~~ & \Sixiv   & Ly$\alpha$  \\
  6.726(.037) & 0.53(.25) &  6.67          & 0.40(.05) &  6.688         & 1.853   & \Sixiii  & He4         \\
  8.295(.028) & 0.13(.07) &  8.43          & 0.14(.04) &  8.315         & 1.491   & \Fexxiv  & Li3-13      \\
  8.424(.032) & 0.17(.08) &                &           &  8.421         & 1.472   & \Mgxii   & Ly$\alpha$  \\
  9.224(.037) & 0.19(.11) &  9.22          & 0.17(.04) &  9.170         & 1.352   & \Mgxi    & He4         \\
  9.412(.050) & 0.16(.11) &                &           &  9.3~~~        & 1.08~~ &  Fe-L    &             \\
 12.136(.064) & 0.32(.22) &  ---           & ---       & 12.134         & 1.022   & \Nex     & Ly$\alpha$  \\
 13.476(.041) & 0.28(.09) &  ---           & ---       & 13.448         & 0.922   & \Neix    & He4         \\
              &           &                &           & 13.467         & 0.921   & \Fexix   & O1-74       \\
 14.251(.028) & 0.20(.09) &  ---           & ---       & 14.260         & 0.869   & \Fexviii & F1-56, 55, 52 \\
 14.974(.021) & 0.30(.09) &  ---           & ---       & 15.013         & 0.826   & \Fexvii  & Ne1-27      \\
 15.236(.032) & 0.14(.08) &  ---           & ---       & 15.265         & 0.812   & \Fexvii  & Ne1-23      \\
 15.989(.032) & 0.14(.07) &  ---           & ---       & 16.002         & 0.775   & \Fexviii & F1-4        \\
 16.791(.023) & 0.19(.08) &  ---           & ---       & 16.780         & 0.738   & \Fexvii  & Ne1-5       \\
 17.115(.069) & 0.08(.07) &  ---           & ---       & 17.055         & 0.727   & \Fexvii  & Ne1-3       \\
              &           &                &           & 17.100         & 0.725   & \Fexvii  & Ne1-2      \\ \hline
\end{tabular}
\begin{flushleft}
{
Notes:
$^a$ Identifications from Kelly (\cite{Kelly87}).
$^b$ Observed average fluxes at Earth in 10$^{-4}$ photon~cm$^{-2}$~s$^{-1}$. No significant
differences between line fluxes of rev.~284 and rev.~285 have been noticed.
$^c$ For notation see Mewe et al.~(\cite{Mewe85}), Phillips et al.~(\cite{Phillips99}), and Note~1
of Sect.~3.2.
}
\end{flushleft}
\end{table}