**Table 2:** Element abundances computed with the MCMC method.
$\begin{displaymath}\begin{tabular}{lcl@{$\,^{+}_{-}\,$}r@{$\,\times\,$}l@{\hspac... ...mes10^{-5}~~$} & \multicolumn{2}{l}{1} \\ \hline \end{tabular}\end{displaymath}$ ^a Number of spectral lines of the relevant element included in the emission measure reconstruction. ^b Element abundance relative to hydrogen. ^c Element abundances relative to the solar ones (Grevesse et al. 1992). ^d Coronal abundance equal to the solar value (Grevesse et al. 1992) as determined by adjustment of the continuum (see Sect. 3.3).

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