All Tables

Table 1: Strongest lines in the Capella spectrum.
Table 2: Element abundances computed with the MCMC method.
Table 3: Density and temperature determination, from the line ratios $R_{\rm D}=f/i$ and $R_{\rm T}=(i+f)/r$ , for the analysed He-like triplets.
Table 4: Results for the short-term variability analysis. We report only upper limits for the effective variability at the 99.7% statistical level, because the emission is compatible with the hypothesis of constant source in the cases.
Table 5: Ascending and descending slope values for the emission measure distributions. The fitting has been performed over the $\log T$ intervals [6.5,6.8] and [6.9,7.2].
Table 6: Volume of coronal plasma at different temperatures evaluated from density values from He-like triplet diagnostics.