All Tables

• Table 1: Observation log for EQ Peg.
• Table 2: Measured line counts and photon fluxes (in 10^-5 photons cm^-2 s^-1) in the combined Chandra MEG spectra. Flux predictions from the reconstructed DEMs (see Sect. 4.2) are also listed.
• Table 3: Measured line counts and photon fluxes in the Chandra MEG spectra of the quiescent state of EQ Peg A.
• Table 4: f/i ratios (in photon units) and coronal densities for EQ Peg A and B from total Chandra MEG spectra.
• Table 5: Absolute coronal abundances (relative to Asplund et al. 2005) of EQ Peg A and B for the total observation time, determined with the DEM methods.
• Table 6: Coefficients for Eqs. (6) and (7) to obtain temperature-independent abundance ratios.
• Table 7: Abundance ratios (relative to Asplund et al. 2005) applying temperature structure-independent linear combinations of coronal emission lines. Values given in brackets for EQ Peg A correspond to the quiescent state.
• Table 8: Abundance ratios relative to Asplund et al. (2005) of EQ Peg A and B, determined from the absolute abundances listed in Table 5.
• Table 9: Properties of active M dwarfs observed with Chandra HETGS. X-ray luminosities are computed from the total background-subtracted counts contained in the MEG spectra from 2-25 Å. Values given in brackets correspond to the quiescent state.
• Table 10: Abundance ratios of other M dwarfs observed with the Chandra HETGS. Values obtained for the quiescent state are given in brackets.