$\begin{figure} \par\mbox{\includegraphics[width=6.5cm,clip]{3752f1_1.ps}\quad \includegraphics[width=6.4cm,clip]{3752f1_2.ps} }\end{figure}$ Figure 1: Peak flux density versus observed peak frequency ( left) and peak luminosity versus rest frame turnover frequency ( right) for GPS galaxies in the various samples. HFP: filled circles; Bolton sample A: $\times$ ; WENSS: filled squares; CORALZ: filled triangles; Stanghellini: $\star$ ; Parkes: +.
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In the text

$\begin{figure} \par\includegraphics[width=6.5cm,clip]{3752fig2.ps} \end{figure}$ Figure 2: Distributions of measured and estimated redshifts for the HFP, Stanghellini et al. (1998), Snellen et al. (1998), Bolton et al. (2004, sample A), Parkes, and ATCA GPS galaxy samples. Note that the peaks at z=1.5 are due to unidentified sources, assumed to be galaxies at that redshift.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=6.5cm,clip]{3752f1_1.ps}\quad \includegraphics[width=6.4cm,clip]{3752f1_2.ps} }\end{figure}$	Figure 1: Peak flux density versus observed peak frequency ( left) and peak luminosity versus rest frame turnover frequency ( right) for GPS galaxies in the various samples. HFP: filled circles; Bolton sample A: $\times$ ; WENSS: filled squares; CORALZ: filled triangles; Stanghellini: $\star$ ; Parkes: +.
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$\begin{figure} \par\includegraphics[width=6.5cm,clip]{3752fig2.ps} \end{figure}$	Figure 2: Distributions of measured and estimated redshifts for the HFP, Stanghellini et al. (1998), Snellen et al. (1998), Bolton et al. (2004, sample A), Parkes, and ATCA GPS galaxy samples. Note that the peaks at z=1.5 are due to unidentified sources, assumed to be galaxies at that redshift.
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$\begin{figure} \par\mbox{\includegraphics[width=4.5cm,clip]{3752f3_1.ps}\qquad \... ...ad \includegraphics[width=4.5cm,clip]{3752f3_5.ps}\hspace*{2.5cm}}\end{figure}$	Figure 3: Spectra of GPS sources in the various samples, normalized in both frequency and flux density.
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$\begin{figure} \par\mbox{\includegraphics[height=4.2cm,clip]{3752f4_1.ps}\qquad ... ...hspace*{4.5mm} \includegraphics[height=4.25cm,clip]{3752f4_6.ps} }\end{figure}$	Figure 4: Comparison of the redshift distributions yielded by the best fit model (dashed) with the observed ones (solid).
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$\begin{figure} \par\mbox{\includegraphics[height=4.2cm,clip]{3752f5_1.ps}\qquad ... ...\hspace*{4.2mm} \includegraphics[height=4.2cm,clip]{3752f5_6.ps} }\end{figure}$	Figure 5: Comparison of the peak frequency distributions yielded by the best fit model (dashed) with the observed ones (solid).
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