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Table 3:

Fluxes and luminosities (first ten entries).

Star 		$f_{\rm [Ne~II]}$a $L_{\rm [Ne~II]}$ $f_{\rm X, 0.3{-}10, abs}$ $L_{\rm X, 0.3{-}10, abs}$ $f_{\rm X, 0.3{-}10, unabs}$ $L_{\rm X, 0.3{-}10, unabs}$ $N_{\rm H}$b Refs.c
  (erg cm-2 s-1) (erg s-1) (erg cm-2 s-1) (erg s-1) (erg cm-2 s-1) (erg s-1) (1022)  
RNO 15 < $2.6(0.85)\phantom{ }\times 10^{-14} $ < $1.9\times 10^{29}$ $3.7\times 10^{-13}$ $2.8\times 10^{30}$ $1.1\times 10^{-12}$ $8.0\times 10^{30}$ 4.6 1, X
LkH$\alpha$ 270 $ 1.3(0.35)\phantom{ }\times 10^{-14} $ $ 9.7\times 10^{28}$ $3.2\times 10^{-13}$ $2.4\times 10^{30}$ $1.5\times 10^{-12}$ $1.1\times 10^{31}$ 0.78 1, X
LkH$\alpha$ 271 < $3.6(1.2)\phantom{0}\times 10^{-15} $ < $2.7\times 10^{28}$ $3.8\times 10^{-14}$ $2.8\times 10^{29}$ $1.1\times 10^{-13}$ $7.9\times 10^{29}$ 3.8 1, X
LkH$\alpha$ 326 $ 3.1(1.4)\phantom{0}\times 10^{-15} $ $ 2.3\times 10^{28}$ ... ... ... ... ... 1
LkH$\alpha$ 327 $ 7.8(3.8)\phantom{0}\times 10^{-15} $ $ 5.8\times 10^{28}$ ... ... ... ... ... 1
LkH$\alpha$ 330 $ 3.8(1.9)\phantom{0}\times 10^{-15} $ $ 2.8\times 10^{28}$ ... ... ... ... ... 1
IRAS 03446+3254 $ 4.3(0.99)\phantom{ }\times 10^{-15} $ $ 3.2\times 10^{28}$ ... ... ... ... ... 1, X
BP Tau $ 2.9(0.4)\phantom{0}\times 10^{-15} $ $ 6.8\times 10^{27}$ $4.3\times 10^{-13}$ $1.0\times 10^{30}$ $6.1\times 10^{-13}$ $1.4\times 10^{30}$ 0.09 3, X
FM Tau < $1.1(0.37)\phantom{ }\times 10^{-14} $ < $2.6\times 10^{28}$ $1.5\times 10^{-13}$ $3.5\times 10^{29}$ $2.2\times 10^{-13}$ $5.1\times 10^{29}$ 0.15 3, X
T Tau N $ 2.0(0.4)\phantom{0}\times 10^{-13} $ $ 4.7\times 10^{29}$ $1.9\times 10^{-12}$ $4.4\times 10^{30}$ $4.0\times 10^{-12}$ $9.4\times 10^{30}$ 0.34 5, X

Notes. (a) Errors are given in parentheses. (b) In units of 1022 cm-2. (c) Reference: 1: New analysis of Spitzer c2d sample, for original analysis see Lahuis et al. (2007); 2: Pascucci et al. (2007); 3: archival GTO/GO observations, see Najita & Carr (in prep.); 4: Herczeg et al. (2007); 5: van Boekel et al. (2009); 6: Espaillat et al. (2007); C: from Chandra archive; X: from XMM-Newton archive.


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