Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig1.ps}\end{figure}$ Figure 1: The V band light curve of 0748+294 on the night of January 13, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig2.ps}\end{figure}$ Figure 2: The V band light curve of 0945+438 on the night of February 26, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig3.ps}\end{figure}$ Figure 3: The V band light curve of 1017+280 on the night of January 14, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig4.ps}\end{figure}$ Figure 4: The V band light curve of 1017+280 on the night of February 27, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig5.ps}\end{figure}$ Figure 5: The V band light curve of 1029+329 on the night of April 05, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig6.ps}\end{figure}$ Figure 6: The V band light curve of 1101+319 on the night of April 04, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig7.ps}\end{figure}$ Figure 7: The V band light curve of 1103-006 on the night of April 06, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig8.ps}\end{figure}$ Figure 8: The V band light curve of 1225+317 on the night of April 07, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.3cm,height=6cm,clip]{2370fig9.ps}\end{figure}$ Figure 9: The V band light curve of 1252+020 on the night of March 09, 2000.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,height=7.7cm,clip]{2370fig10.ps}\end{figure}$ Figure 10: Histogram of observing runs on radio-quiet AGNs. NV, PV and V denote the sources detected: non variable, possible variable and variable respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,height=7.7cm,clip]{2370fig11.ps}\end{figure}$ Figure 11: Histogram of observing runs on radio-loud AGNs (non blazars). NV, PV and V denote the sources detected: non variable, possible variable and variable respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,height=7.7cm,clip]{2370fig12.ps}\end{figure}$ Figure 12: Histogram of observing runs on radio-loud AGNs (blazars). NV, PV and V denote the sources detected: non variable, possible variable and variable respectively.
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In the text