All Tables

Table 1: Log of the XMM-Newton observation.
Table 2: Best-fit models of the EPIC data (in the 1.5-41 Å band), with 90% statistical confidence ranges computed for one interesting parameter at a time; nominal errors on T_i and EM_i are at the 10% level. Element abundances are relative to the solar ones (Grevesse et al. 1992). Mean temperatures are calculated as <T> = $\sum_{i=1}^{3}EM_{i}~T_{i}/\sum_{i=1}^{3}EM_{i}$ .
Table 4: Ratios between elemental and iron coronal abundances, relative to the solar photospheric ratios (Grevesse et al. 1992), derived from RGS data, using the APED and CHIANTI databases; errors are at 68% confidence level. For each element, the number of lines included in the EM reconstruction is also shown.
Table 3: Strongest lines in the spectrum of 31 Com.