All Tables

Table 1: Properties of observations not already described in Ness et al. (2003b).
Table 2: Description of the stellar sample.
Table 3: Measured Fe XXI counts obtained from the available LETGS spectra.
Table 4: Blending prediction of Ne IX intercombination line for HEG (first lines) and MEG (second lines).
Table 5: Coronae with lowest measured f/i ratios (oxygen: f/i <2.2, neon: f/i <2.0). (H = HEG, M = MEG); for neon the predicted blending is taken into account (Sect. 4.3)
Table A.1: X-ray luminosities, H-like and He-like line fluxes, and ion-specific luminosities and emission measures.
Table A.2: Measured line counts for O VII and Ne IX intercombination (i) and forbidden (f) lines, corresponding f/i ratios (corrected for $A_{\rm eff}$ ), and plasma densities $n_{\rm e}$ derived from Eq. (2). All errors are 1 $\sigma$ errors.
Table A.3: Derived volumes $V_{\rm cor}$ in comparison with available volumes $V_{\rm avail}$ .
Table A.4: Same as Table A.1 for RSCVn systems in our sample.
Table A.5: Same as Table A.2 for RSCVn systems in our sample.
Table A.6: Same as Table A.3 for RSCVn systems in our sample.