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Table 1:

CO5BOLD radiation-hydrodynamics model atmospheres.

Model		 $T_{\rm eff}$ \ensuremath{\log g} \ensuremath{[{\rm Fe/H}]} \ensuremath{R} \ensuremath{l_{x}}, \ensuremath{l_{y}} \ensuremath{l_{z}} T $\tau_{\rm c}$ $H_{{\rm p}}^{{\rm surf}}$ \ensuremath{\delta I_{\rm rms}/I} \ensuremath{{\ensuremath{\sigma_{{\rm gran}}}}} $N_{\rm obm}$ Modelcode
  [K] [ ${\rm cm/s^2}$]   [ \ensuremath{{R}_{\hbox{$\odot$ }}}] [Mm] [Mm] [ks] [s] [Mm]   [ppm]    

S0		 6 720 4.25 0.0 1.35 16.4 24.2 135.6 29.5 0.241 0.196 84 (17) 5 d3t68g43mm00n01
S1 6 730 4.25 -1.0 1.35 16.1 24.2 73.8 29.1 0.238 0.229 64 (13) 6 d3t68g43mm10n01
Sun1 5 780 4.44 0.0 1.00 5.6 2.5 52.2 17.8 0.141 0.172 40 (8) 5 d3gt57g44n53
``Model'' is the model's name used in this paper, \ensuremath{T_{{\rm eff}}} the effective temperature, \ensuremath{\log g} the gravitational acceleration, \ensuremath{[{\rm Fe/H}]} the metallicity, \ensuremath{R} an assumed stellar radius (not intrinsic to the simulation proper), $\ensuremath{l_{x}} =\ensuremath{l_{y}} $ the linear horizontal size of the square-shaped computational box, \ensuremath{l_{z}} its vertical extent, T the duration of the simulated time series, \ensuremath{\tau_{\rm c}} the sound crossing time over \ensuremath{H_{\rm P}^{\rm surf}}, \ensuremath{H_{\rm P}^{\rm surf}} the pressure scale height at Rosseland optical depth unity, \ensuremath{\delta I_{\rm rms}/I} the relative spatial white light intensity contrast at disk-center, \ensuremath{{\ensuremath{\sigma_{{\rm gran}}}}} the temporal relative disk-integrated granulation-related brightness fluctuations in white light (in parenthesis an estimate of the uncertainty), $N_{\rm obm}$ the number of equivalent frequency points considered in the solution of the radiative transfer equation, ``Modelcode'' an internal identifier of the model sequence.

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