\begin{table}%t1
\caption{\label{deltas}Far-UV and IR fractions of the unobserved bolometric flux as a function of $T_{\rm eff}$ and $\log g$, the function~$\Lambda(T_{\rm eff},\log g)$, and temperatures~$T_{\rm eff}^f$ as a function of~$T_{\rm eff}(\gamma)$.}
\par
\small%\centerline
 {
\begin{tabular}{c|ccccr|ccccr|ccccr}
\hline
\hline
&\multicolumn{5}{c|}{$\log g = 4.0$} & \multicolumn{5}{c|}{$\log g = 3.0$} &\multicolumn{5}{c}{$\log g = 2.5$}\\
$T_{\rm eff}(\gamma)$ & $\delta^*_{\rm UV}$ &  $\delta^*_{\rm IR}$ & $\Lambda[T_{\rm eff}(\gamma),g]$ & $\gamma$ & $T_{\rm eff}^f$ & $\delta^*_{\rm UV}$ &  $\delta^*_{\rm IR}$ & $\Lambda[T_{\rm eff}(\gamma),g]$ & $\gamma$ & $T_{\rm eff}^f$ &
$\delta^*_{\rm UV}$ &  $\delta^*_{\rm IR}$ & $\Lambda[T_{\rm eff}(\gamma),g]$ & $\gamma$ & $T_{\rm eff}^f$ \\[2pt]
\hline 
10~000&0.023&0.059&0.024&1.5& 9970& 0.024& 0.059& 0.028 & 1.5 &  9970 & 0.023 & 0.059 & 0.029 & 1.5 &  9960 \\
     &     &     &     &2.0& 9940&      &      &       & 2.0 &  9930 &       &       &       & 2.0 &  9930 \\
12~500&0.105&0.034&0.088&1.5&12~360& 0.099& 0.034& 0.086 & 1.5 & 12~360 & 0.093 & 0.034 & 0.081 & 1.5 & 12~370 \\
     &     &     &     &2.0&12~220&      &      &       & 2.0 & 12~220 &       &       &       & 2.0 & 12~240 \\
15~000&0.230&0.022&0.152&1.5&14~710& 0.218& 0.022& 0.135 & 1.5 & 14~740 & 0.202 & 0.022 & 0.122 & 1.5 & 14~770 \\
     &     &     &     &2.0&14~390&      &      &       & 2.0 & 14~470 &       &       &       & 2.0 & 14~520 \\
17~500&0.386&0.016&0.182&1.5&17~090& 0.353& 0.016& 0.155 & 1.5 & 17~150 & 0.318 & 0.016 & 0.134 & 1.5 & 17~200 \\
     &     &     &     &2.0&16~640&      &      &       & 2.0 & 16~780 &       &       &       & 2.0 & 16~880 \\
20~000&0.552&0.012&0.194&1.5&19~450& 0.484& 0.012& 0.157 & 1.5 & 19~600 & 0.450 & 0.012 & 0.135 & 1.5 & 19~650 \\
     &     &     &     &2.0&18~950&      &      &       & 2.0 & 19~160 &       &       &       & 2.0 & 19~290 \\
22~500&0.706&0.009&0.191&1.5&21~940& 0.596& 0.010& 0.139 & 1.5 & 22~090 & 0.546 & 0.010 & 0.109 & 1.5 & 22~190 \\
     &     &     &     &2.0&21~340&      &      &       & 2.0 & 21~670 &       &       &       & 2.0 & 21~860 \\
25~000&0.843&0.008&0.178&1.5&24~420& 0.693& 0.008& 0.106 & 1.5 & 24~670 & 0.635 & 0.008 & 0.071 & 1.5 & 24~780 \\
     &     &     &     &2.0&23~800&      &      &       & 2.0 & 24~310 &       &       &       & 2.0 & 24~540 \\
27~500&0.955&0.007&0.153&1.5&26~950& 0.823& 0.007& 0.093 & 1.5 & 27~180 &       &       &       &     &       \\
     &     &     &     &2.0&26~380&      &      &       & 2.0 & 26~840 &       &       &       &     &       \\
30~000&1.060&0.006&0.126&1.5&29~520& 1.023& 0.006& 0.087 & 1.5 & 29~670 &       &       &       &     &       \\
     &     &     &     &2.0&29~010&      &      &       & 2.0 & 29~330 &       &       &       &     &       \\
32~500&1.241&0.005&0.109&1.5&32~050&      &      &       &     &       &       &       &       &     &       \\
     &     &     &     &2.0&31~580&      &      &       &     &       &       &       &       &     &       \\
35~000&1.539&0.004&0.103&1.5&34~540&      &      &       &     &       &       &       &       &     &       \\
     &     &     &     &2.0&34~060&      &      &       &     &       &       &       &       &     &       \\
\hline
\end{tabular}}
\medskip
For $\Lambda(T_{\rm eff})$ and $T_{\rm eff}$ the temperature $T_{\rm eff}(\gamma)$ is simply the effective temperature written in the first column of the table. \\
Parameters $\delta^*_{\rm UV}$ and $\delta^*_{\rm IR}$ are values of  $\delta_{\rm UV}$ and $\delta_{\rm IR}$ calculated with $T_{\rm eff}(\gamma)$ and fluxes $F_{\lambda}[T_{\rm eff}(\gamma),\log g]$, which do not undergo the transformation given by Eq.~(\ref{gama}). To calculate them we have used $\lambda_a=1380$~\AA\ and $\lambda_b=11~084$~\AA. Note that $T^f_{\rm eff}=$ $T_{\rm eff}(\gamma=1)$.
\end{table}