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\begin{table} \caption{\label{tabmod}Details of the 3D hydrodynamical model atmospheres.} %\centerline {\begin{tabular}{lrrrr} \hline \hline \noalign{\smallskip} $\langle T_{\rm eff} \rangle$$^a$ & $\log{g}$ & [Fe/H] & Time$^b$ & Snapshots \\ \noalign{\smallskip} [K] & [cgs] & [dex] & [s] & \\ \noalign{\smallskip} \hline \noalign{\smallskip} 5500 & 3.5 & --2 & 46~800 & 20 \\ % 46800.0 5470 & 4.0 & --2 & 33~800 & 20 \\ % 33800.0 5480 & 4.5 & --2 & 57~000 & 20 \\ % 57000.0 5860 & 3.5 & --2 & 112~000 & 20 \\ % 112000.0 5860 & 4.0 & --2 & 30~000 & 20 \\ % 30000.0 5920 & 4.5 & --2 & 24~500 & 18 \\ % 24499.9 6290 & 3.5 & --2 & 82~800 & 18 \\ % 92000.0 for 20 snapshots 6280 & 4.0 & --2 & 27~600 & 16 \\ % 27600.3 6320 & 4.5 & --2 & 9100 & 19 \\ % 9119.95 6530 & 4.0 & --2 & 49~200 & 20 \\ % 49200.0 6530 & 4.5 & --2 & 9100 & 19 \\ \hline \end{tabular}} \smallskip \par $^{a}$ Temporal average of the emergent \teffo. $^{b}$ Total time covered by the temporal evolution of the photospheric flow sampled at equal intervals in time named as snapshots. \par \end{table}