All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f1} \end{figure}$ Figure 1: Classical, current, and future concepts for adding and editing catalogue data in comparison.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f2} \end{figure}$ Figure 2: Search form in CVcat: A large fraction of the search form focuses on the detailed selection of the object class.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f3} \end{figure}$ Figure 3: Search result in CVcat: Some of the data stored for SS Cygni.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{3352f4.eps} \end{figure}$ Figure 4: Secondary mass plotted against orbital period (points) and period histogram (gray bars) for all CVs with known orbital period and secondary mass. The full line shows the relation from Eq. (1), the short dashed line from Eq. (3), the long dashed line from Eq. (4). Full boxes and error bars are used for systems with estimated errors in M₂, open boxes for secondary star masses with an unknown error range. The given (M₂,P) data pairs represent $\approx$ 10% of all known CVs, the histogram contains $\approx$ $39\%$ of all CVs known to CVcat.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f1} \end{figure}$	Figure 1: Classical, current, and future concepts for adding and editing catalogue data in comparison.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f2} \end{figure}$	Figure 2: Search form in CVcat: A large fraction of the search form focuses on the detailed selection of the object class.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3352f3} \end{figure}$	Figure 3: Search result in CVcat: Some of the data stored for SS Cygni.
Open with DEXTER