All Tables

Table 1: Results of the joint MOS1 and MOS2 spectral fits of SU Aur. The intervals for time-dependent analysis are indicated in Fig. 2. Errors are computed with $\Delta \chi ^2=1$ , allowing all parameters to vary. When no error is given, the parameter was kept fixed to the tabulated value.
Table 3: X-ray properties of known Taurus-Auriga members and of other stars detected in our observation. For the last three members we give the position of the nearest X-ray source, even if its distance is greater than 4 $^{\prime \prime }$ .
Table 4: Best-fit parameters for the quiescent and flaring spectra of HD 31305. Errors are as in Table 1.
Table 2: Strongest lines measured in the RGS spectrum of SU Aur. Only lines with $S/N \ge 1.5$ are listed. Asterisks mark the lines used for the EM reconstruction. $\lambda _{\rm obs}$ is the measured wavelenght, $\lambda _{\rm pred}$ is the theoretical wavelenght of the transition, and $T_{\rm max}$ is the temperature of maximum emissivity in K.