$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig1.ps} \end{figure}$ Figure 1: Ultraviolet energy distribution of HS 1700+6416 [10^-15 erg s^-1 cm^-2 Å^-1] for selected epochs (cf. Table 1).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig2.ps} \end{figure}$ Figure 2: Light curve of HS 1700+6416 from the Hamburg Quasar monitoring program (Borgeest & Schramm 1994). The dates of (quasi) simultaneous UV observations are indicated.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig3.ps} \end{figure}$ Figure 3: Flux at 1250 Å (in units of $1.1 \times 10^{-15}$ erg s^-1 cm^-2 Å^-1) versus R band flux (in units of $7.5 \times 10^{-16}$ erg s^-1 cm^-2 Å^-1).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig1.ps} \end{figure}$	Figure 1: Ultraviolet energy distribution of HS 1700+6416 [10^-15 erg s^-1 cm^-2 Å^-1] for selected epochs (cf. Table 1).
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$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig2.ps} \end{figure}$	Figure 2: Light curve of HS 1700+6416 from the Hamburg Quasar monitoring program (Borgeest & Schramm 1994). The dates of (quasi) simultaneous UV observations are indicated.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{2303fig3.ps} \end{figure}$	Figure 3: Flux at 1250 Å (in units of $1.1 \times 10^{-15}$ erg s^-1 cm^-2 Å^-1) versus R band flux (in units of $7.5 \times 10^{-16}$ erg s^-1 cm^-2 Å^-1).
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