Table 1: Parameters adopted for the construction of the Doppler images of BO Mic, $\epsilon $ represents the linear limb darkening coefficient. The spot continuum flux is given relative to an undisturbed photospheric continuum flux of one. Note that the given margins designate the deviations between parameters adopted for different reconstructions, they are not proper error estimates.

Rotation period
P0=0.380 days
Inclination 70 $\hbox{$^\circ$ }$
Spot continuum flux 0.5
$v~\sin{i}$ $134\pm2$ km s-1
$\epsilon $ $0.9\pm0.1$ ("6120 Å'')
  $0.7\pm0.1$ ("6400 Å'')

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