Table 2: Absolute coronal abundances of CN Leo1.
  C N O Ne Mg Si S Fe
XSPEC 1.49 $\pm$ 0.24 1.28 $\pm$ 0.21 0.62 $\pm$ 0.08 1.20 $\pm$ 0.16 0.85 $\pm$ 0.17 0.78 $\pm$ 0.33 1.41 $\pm$ 0.27 0.59 $\pm$ 0.07
$\it DEM$ method 1 1.27 $\pm$ 0.13 1.03 $\pm$ 0.13 0.66 $\pm$ 0.03 1.22 $\pm$ 0.11 0.92 $\pm$ 0.16 n.a. n.a 0.56 $\pm$ 0.04
$\it DEM$ method 2 1.18 $\pm$ 0.12 0.97 $\pm$ 0.12 0.63 $\pm$ 0.03 1.17 $\pm$ 0.11 0.85 $\pm$ 0.15 n.a. n.a 0.55 $\pm$ 0.04
1 Abundances are derived from the RGS and EPIC data as fitted with a three component temperature model as described in Sect. 4.1. Methods 1 and 2 use a differential emission measure method as described in Sect. 4.2. The given errors are the statistical 1$\sigma$ standard deviations.

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