$\begin{figure} \par\includegraphics[width=18.0cm,clip]{MS3459f1.ps}\end{figure}$ Figure 1: PHOT-S spectra of the four galaxies. On the left, the two "starburst'' galaxies, IRAS 14201+2956 and IRAS 21582+1018 (alias Mrk 520); on the right, the two NLS1 objects, Mrk 359 and Mrk 1388. Tickmarks indicate the detected lines.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{MS3459f3.ps}\end{figure}$ Figure 3: Low dispersion spectrum of IRAS 14201+2956 obtained in May 92. Note the absence of conspicuous Seyfert features.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{MS3459f4.ps}\end{figure}$ Figure 4: Low dispersion spectrum of IRAS 21582+1018 obtained in Sep. 96. No broad Aline features are apparent, but line ratios are close to the borderline between AGN and HII type galaxies.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{MS3459f5.ps}\end{figure}$ Figure 5: IRAS 21582+1018 high dispersion spectrum (Sep. 96) in the H $_{\alpha }$ region. The presence of a broad H $_{\alpha }$ component can only be established by multi-component fiting (dashed lines).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.85cm,clip]{MS3459f6.ps}\end{figure}$ Figure 6: IRAS 14201+2956 high dispersion spectrum (May 1998) in the H $_{\alpha }$ region. The result of multi-component fiting is shown with dashed-lines.
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In the text

$\begin{figure} \par\includegraphics[width=18.0cm,clip]{MS3459f1.ps}\end{figure}$	Figure 1: PHOT-S spectra of the four galaxies. On the left, the two "starburst'' galaxies, IRAS 14201+2956 and IRAS 21582+1018 (alias Mrk 520); on the right, the two NLS1 objects, Mrk 359 and Mrk 1388. Tickmarks indicate the detected lines.
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$\begin{figure} \par\includegraphics[height=7.0cm,width=7cm,angle=-90,clip]{MS3459f2.ps}\end{figure}$	Figure 2: Individual Neon lines detected in IRAS 21582+1018.
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$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{MS3459f3.ps}\end{figure}$	Figure 3: Low dispersion spectrum of IRAS 14201+2956 obtained in May 92. Note the absence of conspicuous Seyfert features.
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$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{MS3459f4.ps}\end{figure}$	Figure 4: Low dispersion spectrum of IRAS 21582+1018 obtained in Sep. 96. No broad Aline features are apparent, but line ratios are close to the borderline between AGN and HII type galaxies.
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$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{MS3459f5.ps}\end{figure}$	Figure 5: IRAS 21582+1018 high dispersion spectrum (Sep. 96) in the H $_{\alpha }$ region. The presence of a broad H $_{\alpha }$ component can only be established by multi-component fiting (dashed lines).
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$\begin{figure} \par\includegraphics[angle=-90,width=7.85cm,clip]{MS3459f6.ps}\end{figure}$	Figure 6: IRAS 14201+2956 high dispersion spectrum (May 1998) in the H $_{\alpha }$ region. The result of multi-component fiting is shown with dashed-lines.
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$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{MS3459f7.ps}\end{figure}$	Figure 7: Low dispersion spectrum of Mrk 359 (January 96).
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$\begin{figure} \par\includegraphics[angle=-90,width=7.7cm,clip]{MS3459f8.ps}\end{figure}$	Figure 8: Low dispersion spectrum of Mrk 1388 (June 99).
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