Table 1: Parameters of the underlying photospheres for the model construction. From the literature we also cite [A/H] given in brackets.
Star Other name Spectrum used $T_{{\rm eff}}$ [K] log g Literature
AD Leo GJ 388 2002-03-16 03:40:47 3200 4.5 3350, 4.5 (-0.75) 1
YZ CMi GJ 285 average 3000 4.5 2925 3
CN Leo GJ 406 2002-03-14 03:24:38 2900 5.5 2900, 5.0 (0.0) 1
DX Cnc GJ 1111 average 2700 5.0 2850, 5.25 (+0.5) 1; 2775 3
LHS 3003 GJ 3877 average 2500 4.5 2400-2650 2
$\textstyle \parbox{13cm}{ $^{1}$\space \citet{Jones}, $^{2}$\space \citet{Leggett}, $^{3}$\space \citet{Mohanty}.}$

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observations and data analysis
3 Model construction and calculation
4 The influence of the model parameters
5 Results
6 Discussion
7 Summary and conclusion
References
Online Material
Appendix A: Identification of chromospheric emission lines
List of tables
List of figures