All Figures

$\begin{figure} \par\includegraphics[height=8.15cm,width=8.25cm,clip]{1772fig1.ps}\end{figure}$ Figure 1: Light curve of 3EG J0416+3650 from April 1991 to September 1995.
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In the text

$\begin{figure} \par\includegraphics[height=8.8cm,width=8.8cm,clip]{1772fig2.ps}\end{figure}$ Figure 2: The BeppoSAX-MECS (2-10 keV) image superimposed on the EGRET $\gamma$ -ray probability contours at 50%, 68%, 95%, 99% and 99.9% confidence level.All sources listed in Tables 1 and 3 are shown: crosses are ROSAT Faint sources, diamond is Einstein Slew Survey source, pluses are NVSS radio sources and squares are Green Bank radio sources.
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In the text

$\begin{figure} \par\includegraphics[height=7.25cm,width=8.05cm,clip]{1772fig3.ps}\end{figure}$ Figure 3: The observed SED of 3C 111. We shown here all published data. Open circles are radio measurements, open squares are millimeter measurements, filled triangles are IRAS data, open pentagons are 2MASS measurements (bands J, H, K), filled circles are optical measurements (bands I, V, B), filled squares are our BeppoSAX measurements, open triangles are EGRET measurementsa and arrows are 2 $\sigma$ COMPTEL upper limits (0.75-1 MeV, 1-3 MeV, 3-10 MeV).
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In the text

$\begin{figure} \par\includegraphics[height=7.25cm,width=8.05cm,clip]{1772fig4.ps}\end{figure}$ Figure 4: The corrected SED of 3C 111. Optical and far-infrared data points(filled circles and open pentagons, respectively) have been dereddened with $A_{\rm V}$ = 1.3, while the X-ray point at 2 keV has been corrected for $N_{\rm H}$ = 1.2 $\times$ 10²² cm^-2.
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In the text

$\begin{figure} \par\includegraphics[height=8.15cm,width=8.25cm,clip]{1772fig1.ps}\end{figure}$	Figure 1: Light curve of 3EG J0416+3650 from April 1991 to September 1995.
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$\begin{figure} \par\includegraphics[height=8.8cm,width=8.8cm,clip]{1772fig2.ps}\end{figure}$	Figure 2: The BeppoSAX-MECS (2-10 keV) image superimposed on the EGRET $\gamma$ -ray probability contours at 50%, 68%, 95%, 99% and 99.9% confidence level.All sources listed in Tables 1 and 3 are shown: crosses are ROSAT Faint sources, diamond is Einstein Slew Survey source, pluses are NVSS radio sources and squares are Green Bank radio sources.
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$\begin{figure} \par\includegraphics[height=7.25cm,width=8.05cm,clip]{1772fig4.ps}\end{figure}$	Figure 4: The corrected SED of 3C 111. Optical and far-infrared data points(filled circles and open pentagons, respectively) have been dereddened with $A_{\rm V}$ = 1.3, while the X-ray point at 2 keV has been corrected for $N_{\rm H}$ = 1.2 $\times$ 10²² cm^-2.
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