All Figures

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{0152fig1.ps} \end{figure}$ Figure 1: Aitoff projection of the observed sample in J2000 equatorial coordinates, histogram of radial velocities V₂₀ and HI fluxes (see Table 2).
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In the text

$\begin{figure} \par\includegraphics[width=17cm]{0152fig2.eps} \end{figure}$ Figure 2: Summary of template radiosource flux measurement in period 2001-2002. The four panels show the mean value of the observed fluxes for the 23 templates as a function of date for two frequencies (1380 MHz and 1410 MHz) and two polarization (E and W).
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0152fig3.ps} \end{figure}$ Figure 3: Gain curve of the antenna as a function of declination.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{0152fig4.ps} \end{figure}$ Figure 4: Upper panel: distribution of integration time per galaxy in units of ON/OFF cycles number. Lower panel: rms noise $\sigma$ in mJy as a function of integration time expressed in number of integration cycles; the solid line is the function $24.5 / \sqrt {N_{\rm cy}}$ .
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0152fig5.ps} \end{figure}$ Figure 5: Projection of the major axis D₂₅ on the East-West direction.
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In the text

$\begin{figure} \par\includegraphics[width=15.5cm,clip]{0152fig6.ps} \end{figure}$ Figure 6: Evolution of the normalized HI-flux ( $F_{\rm HI}/F_0$ ) and rms noise in the baseline for our 58 template galaxies during the survey: a) template galaxies with $F_{\rm HI} > 17$ Jy km s^-1, the dashed lines shows the 1.5 $\sigma$ levels, b) template galaxies with $F_{\rm HI} < 17$ Jy km s^-1, c) rms noise $\times$ $\sqrt {N_{\rm cy}}$ , i.e. rms noise for one single cycle of ON/OFF integration, for all template galaxy measurements.
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In the text

$\begin{figure} \par\includegraphics[width=16cm,clip]{0152fig7.ps} \end{figure}$ Figure 7: -excerpt. 21-cm line profiles of galaxies listed in Table 2; profiles are classified according to their PGC name appearing in the top right corner of each panel. The usual name of the galaxy (NGC, UGC, IC, ESO, MCG...) is written above each panel. Ordinate and abscissae axes are graduated respectively in km s^-1 and mJy. Note that heliocentric radial velocities are expressed in terms of optical redshift $c \frac{\Delta \lambda}{\lambda}$ . The horizontal line represents the baseline of the profile, from which the maximum is estimated.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{0152fig1.ps} \end{figure}$	Figure 1: Aitoff projection of the observed sample in J2000 equatorial coordinates, histogram of radial velocities V₂₀ and HI fluxes (see Table 2).
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$\begin{figure} \par\includegraphics[width=17cm]{0152fig2.eps} \end{figure}$	Figure 2: Summary of template radiosource flux measurement in period 2001-2002. The four panels show the mean value of the observed fluxes for the 23 templates as a function of date for two frequencies (1380 MHz and 1410 MHz) and two polarization (E and W).
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$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0152fig3.ps} \end{figure}$	Figure 3: Gain curve of the antenna as a function of declination.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{0152fig4.ps} \end{figure}$	Figure 4: Upper panel: distribution of integration time per galaxy in units of ON/OFF cycles number. Lower panel: rms noise $\sigma$ in mJy as a function of integration time expressed in number of integration cycles; the solid line is the function $24.5 / \sqrt {N_{\rm cy}}$ .
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$\begin{figure} \par\includegraphics[angle=270,width=8.5cm,clip]{0152fig5.ps} \end{figure}$	Figure 5: Projection of the major axis D₂₅ on the East-West direction.
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