Table 3: Target stars: results from the EPIC spectral fits.

Stars		 $N_{\rm H}$ T0 $\beta $ EM1 $T_{\rm av}$ $L_{\rm X}^2$
  ( $10^{22}~\rm {cm}^{-2}$) (MK)   ( $10^{52}~\rm {cm}^{-3}$) (MK) ( $10^{30} \rm {erg~s^{-1}}$)
HD 283572 0.08 (0.07, 0.08) 10.4 (10.0, 10.7) -0.94 (-1.02, -0.87) 114.3 14.4 13.0
V 773 Tau 0.17 (0.17, 0.17) 8.7 (8.4, 9.1) -0.87 (-0.93, -0.82) 89.8 13.0 9.5
V 410 Tau 0.02 (0.02, 0.03) 10.4 (9.4, 10.8) -1.17 (-1.28, -0.96) 44.5 13.2 4.7
HP Tau/G2 0.41 (0.39, 0.42) 9.2 (8.6, 9.9) -1.37 (-1.46, -1.28) 94.6 11.0 9.7
SU Aur 0.47 (0.43 0.48) 6.4 (6.2, 7.6) -1.11 (-1.21, -1.06) 95.4 8.9 9.5
DH Tau 0.20 (0.19, 0.21) 11.5 (11.0, 12.1) -1.38 (-1.49, -1.26) 80.6 13.4 8.5
BP Tau 0.06 (0.06, 0.07) 7.1 (6.7, 7.6) -0.67 (-0.73, -0.60) 12.8 12.3 1.4
DN Tau 0.07 (0.07, 0.08) 10.5 (9.5, 11.5) -1.25 (-1.51, -1.02) 11.0 12.9 1.1
AB Aur 0.05 (0.03, 0.07) 4.8 (4.3, 5.5) -1.55 (-1.78, -1.41) 3.8 5.7 0.4
1 Total EM integrated over temperature bins between $\log T = 6{-}7.9$ [K] (see Güdel et al. 2007a for more details).
2 Calculated in the range 0.3-10 keV.

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