All Figures

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig1.eps}\end{figure}$ Figure 1: Histogram of the mean reddening deviations $\Delta E(B-V)$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig2.eps}\end{figure}$ Figure 2: Histogram of the temperature deviations for CP1 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ).
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{0325fig3.eps}\end{figure}$ Figure 3: The upper panel shows the comparison of the reddening free Strömgren index [u-b] to $\theta _{\rm eff}$ . The line represents the quadratic fit given by Lipski & Stepien (2008). the cool stars also are included, although they are not calibratable via the reddening free index. The lower panel shows the discrepancy of the temperatures determined by the authors to our averaged ones without their results. The line gives the one-to-one relation.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig4.eps}\end{figure}$ Figure 4: Histogram of the temperature deviations for CP2 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ).
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig5.eps}\end{figure}$ Figure 5: Comparison of temperatures determined via ${\it Geneva}$ photometry to literature values for the restricted CP3 and CP4 samples. The upper line shows the one-to-one relation, the middle one our linear fit, and the bottom line the CP2 relation for comparison. Additionally, the outstanding object HD 137509 is given. The error bars correspond to the standard deviation of the average effective temperatures.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig6.eps}\end{figure}$ Figure 6: Histogram of the temperature deviations for CP3 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ). The dark grey portion represents the ``classical'' HgMn objects.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig7.eps}\end{figure}$ Figure 7: Histogram of the temperature deviations for CP4 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ). The dark grey portion represents the He-weak objects.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0325fig8.eps}\end{figure}$ Figure 8: Bolometric corrections for CP stars together with our fit (solid black line) and the relations for normal stars by Balona (1994) and Flower (1996). For better presentation, the comparison of our fit to Lipski & Stepien (2008) and Landstreet et al. (2007) is shifted by -0.6 mag. Whenever available, the error of BC according to error propagation using the standard deviation of the averaged integrated fluxes and 0.02 mag in reddening is given. Additionally the standard deviation of the averaged temperatures is shown.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig1.eps}\end{figure}$	Figure 1: Histogram of the mean reddening deviations $\Delta E(B-V)$ .
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig2.eps}\end{figure}$	Figure 2: Histogram of the temperature deviations for CP1 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ).
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig4.eps}\end{figure}$	Figure 4: Histogram of the temperature deviations for CP2 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ).
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig6.eps}\end{figure}$	Figure 6: Histogram of the temperature deviations for CP3 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ). The dark grey portion represents the ``classical'' HgMn objects.
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$\begin{figure} \par\includegraphics[width=7.6cm,clip]{0325fig7.eps}\end{figure}$	Figure 7: Histogram of the temperature deviations for CP4 stars ( $T_{\rm eff} - \overline {T}_{\rm phot}$ ). The dark grey portion represents the He-weak objects.
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