$\begin{figure} \par\epsfxsize=8.8cm \epsfbox{lumifun.eps}\end{figure}$ Figure 4: Normalized luminosity function of systems with an early type VLG (red squares) and a late type VLG (blue triangles), with Poissonian $1 \sigma$ error bars.
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In the text

$\begin{figure} \par\mbox{\epsfxsize=5.1cm \epsfbox{hisVLG014.eps}\hskip 0.1cm ... ...ace{5.2cm}\epsfxsize=5.1cm \epsfbox{hisVLG109.eps}\hspace{5.2cm}} \end{figure}$	Figure 3: Redshift histograms of the VLG systems with $\ge$ 10 redshifts (dashed line: VLG redshift).
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$\begin{figure} \par\epsfxsize=8.8cm \epsfbox{lumifun.eps}\end{figure}$	Figure 4: Normalized luminosity function of systems with an early type VLG (red squares) and a late type VLG (blue triangles), with Poissonian $1 \sigma$ error bars.
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$\begin{figure} \par\centerline {\hskip 3cm VLG061: finding chart. \hskip 6.6cm ... ...VLG074.eps}\hskip 1cm \epsfxsize=8.0cm \epsfbox{tvVLGN07+53.eps} } \end{figure}$	Figure 1: Finding charts of the VLG fields observed at OHP (the scale is approximately $30 \times 30$ square arcmin).
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$\begin{figure} \par\centerline {\hskip 3.5cm VLG014 \hskip 7.1cm VLG022} \mbox... ...x{VLG043.eps}\hskip 1cm \epsfxsize=8.0cm \epsfbox{VLG045.eps} } \end{figure}$	Figure 2: Finding charts of the VLG fields selected from the 2dFGRS (the scale is approximately $40 \times 30$ square arcmin).
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