All Figures

$\begin{figure} \par\includegraphics[width=18cm,clip]{0562fig1.eps}\end{figure}$ Figure 1: Light curves of several bursts detected by MCAL. Panels a) to c): GRBs triggered on the ground by SRM data. Panels d) to k): GRBs triggered by the on-board logic.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig2.eps} \end{figure}$ Figure 2: Positions of the GRBs detected by MCAL and localized either by Swift (stars), IPN (circles), or SuperAGILE (triangle) in the reference frame of AGILE pointing. The radial coordinate is the off-axis angle with respect to the pointing of the satellite. The thick solid circles represent the GRID and SuperAGILE (the innermost) fields of view.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig3.eps} \end{figure}$ Figure 3: MCAL sensitivity as a function of the peak energy for $40^{\circ }$ off axis GRBs with different Band spectral models. Continuous line: $\alpha =-1$ , $\beta =-2.5$ ; dashed line $\alpha =-0.5$ , $\beta =-2$ ; dot-dashed line $\alpha =-1$ , $\beta =-3$ . Solid triangles: GRBs detected by MCAL at incident angle < $90^\circ$ . Solid circles: GRBs detected by MCAL at incident angle > $90^\circ$ . Hollow triangle: GRB at incident angle < $90^\circ$ but not detected by MCAL.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig4.eps}\end{figure}$ Figure 4: MCAL count spectra for GRB 080407B. Filled triangles: upper detection layer SRM count spectrum. Crosses: count spectrum obtained from photon-by-photon data relative to the whole MCAL.
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In the text

$\begin{figure} \par\begin{tabular}{c} \includegraphics[width=9cm,clip]{0562fig5.eps} \end{tabular}\par \end{figure}$ Figure 5: MCAL total effective area as a function of energy, for different incident angles. Solid line: on-axis beam. Pluses: $40^{\circ }$ off-axis beam. Crosses: $80^\circ$ off-axis beam.
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In the text

$\begin{figure} \par\includegraphics[height=8.8cm, angle=-90]{0562fig6.eps}\end{figure}$ Figure 6: Spectral fitting of GRB 080514B. Filled triangles: MCAL data. Solid line: best fit power law model.
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In the text

$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig7.eps}\end{figure}$ Figure 7: Light curve of the event triggered on 2008-03-23 at 02:28:25 UT.
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In the text

$\begin{figure} \par\includegraphics[width=18cm,clip]{0562fig1.eps}\end{figure}$	Figure 1: Light curves of several bursts detected by MCAL. Panels a) to c): GRBs triggered on the ground by SRM data. Panels d) to k): GRBs triggered by the on-board logic.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig2.eps} \end{figure}$	Figure 2: Positions of the GRBs detected by MCAL and localized either by Swift (stars), IPN (circles), or SuperAGILE (triangle) in the reference frame of AGILE pointing. The radial coordinate is the off-axis angle with respect to the pointing of the satellite. The thick solid circles represent the GRID and SuperAGILE (the innermost) fields of view.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig4.eps}\end{figure}$	Figure 4: MCAL count spectra for GRB 080407B. Filled triangles: upper detection layer SRM count spectrum. Crosses: count spectrum obtained from photon-by-photon data relative to the whole MCAL.
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$\begin{figure} \par\begin{tabular}{c} \includegraphics[width=9cm,clip]{0562fig5.eps} \end{tabular}\par \end{figure}$	Figure 5: MCAL total effective area as a function of energy, for different incident angles. Solid line: on-axis beam. Pluses: $40^{\circ }$ off-axis beam. Crosses: $80^\circ$ off-axis beam.
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$\begin{figure} \par\includegraphics[height=8.8cm, angle=-90]{0562fig6.eps}\end{figure}$	Figure 6: Spectral fitting of GRB 080514B. Filled triangles: MCAL data. Solid line: best fit power law model.
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$\begin{figure} \par\includegraphics[width=9cm,clip]{0562fig7.eps}\end{figure}$	Figure 7: Light curve of the event triggered on 2008-03-23 at 02:28:25 UT.
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