**Table 1:** Strongest lines in the Capella spectrum.
$\begin{displaymath}{\scriptsize \begin{tabular}[h]{@{\hspace{4mm}}l@{\hspace{4mm... ... & $\pm$ & 12 & 58 & $\pm$ & 10 & AB \\ \hline \end{tabular}} \end{displaymath}$ ^a Observed (for each order of the spectrum taken in 2000) and predicted (CHIANTI database) wavelengths in Å. In the cases of unresolved blends, identified by the same label number, we list the main components in order of increasing predicted wavelength. ^b Temperature of maximum emissivity in K. ^c Total line counts for each observation. In the cases of unresolved blends, identified by the same label number, we report only the total line counts. ^d Lines selected to derive the emission measure distribution for the observation taken in 2000 (A) or 2001 (B).

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