$\begin{figure} \par\includegraphics[width=8.8cm,clip]{integral72_f1.ps} \end{figure}$ Figure 1: Bottom: historical light curve of Aql X-1 in the 2-12 keV energy band, obtained by RXTE (data averaged over 1-day intervals). Top: detailed profile of the March, 2003 outburst. Vertical lines indicate moments of the INTEGRAL observations.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{integral72_f21.ps}\par\vspace*{2mm} \includegraphics[width=8.4cm,clip]{integral72_f22.ps} \end{figure}$ Figure 2: X-ray images of the Aql X-1 sky region, obtained with ISGRI/IBIS in the 25-50 keV energy band (upper panel) and JEM-X in the 3-10 keV energy band (bottom panel) in March-April 2003. Contours on the ISGRI/IBIS map are given at the signal-to-noise levels of 2, 2.5, 3.3, 4.5, 6.2,... 42 $\sigma$ (for the brightest sources GRS 1915+105 and X1901+03 contours begin from 4.5 $\sigma$ ).
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{integral72_f3.ps} \end{figure}$ Figure 3: The photon spectra of Aql X-1 observed with INTEGRAL on March 10 (the 1st set of observations) and on April 5 (the 5th set). The best fit thermal bremsstrahlung models are shown by solid lines.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{integral72_f42.ps}\par\vspace*{3mm} \includegraphics[width=7.7cm,clip]{integral72_f41.ps} \end{figure}$ Figure 4: Top: JEM-X light curves containing two X-ray bursts from Aql X-1. Time resolution is 1 s. The zero time on the horizontal axis corresponds to Apr. 5.00 2003 UT. Bottom: image reconstruction of the Aql X-1 field before the burst (1) and during the burst (2).
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{integral72_f5.ps} \end{figure}$ Figure 5: Average photon spectrum of X1901+03 measured with JEM-X and IBIS/ISGRI over the entire set of observations. Solid line shows the approximation by a power law with the high energy cutoff.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{integral72_f7.ps} \end{figure}$ Figure 7: Average photon spectra of XTE J1908+094, X1908+075 and 4U1907+097 obtained with the ISGRI instrument. Solid lines show the power law approximations.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{integral72_f1.ps} \end{figure}$	Figure 1: Bottom: historical light curve of Aql X-1 in the 2-12 keV energy band, obtained by RXTE (data averaged over 1-day intervals). Top: detailed profile of the March, 2003 outburst. Vertical lines indicate moments of the INTEGRAL observations.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{integral72_f21.ps}\par\vspace*{2mm} \includegraphics[width=8.4cm,clip]{integral72_f22.ps} \end{figure}$	Figure 2: X-ray images of the Aql X-1 sky region, obtained with ISGRI/IBIS in the 25-50 keV energy band (upper panel) and JEM-X in the 3-10 keV energy band (bottom panel) in March-April 2003. Contours on the ISGRI/IBIS map are given at the signal-to-noise levels of 2, 2.5, 3.3, 4.5, 6.2,... 42 $\sigma$ (for the brightest sources GRS 1915+105 and X1901+03 contours begin from 4.5 $\sigma$ ).
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{integral72_f3.ps} \end{figure}$	Figure 3: The photon spectra of Aql X-1 observed with INTEGRAL on March 10 (the 1st set of observations) and on April 5 (the 5th set). The best fit thermal bremsstrahlung models are shown by solid lines.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{integral72_f42.ps}\par\vspace*{3mm} \includegraphics[width=7.7cm,clip]{integral72_f41.ps} \end{figure}$	Figure 4: Top: JEM-X light curves containing two X-ray bursts from Aql X-1. Time resolution is 1 s. The zero time on the horizontal axis corresponds to Apr. 5.00 2003 UT. Bottom: image reconstruction of the Aql X-1 field before the burst (1) and during the burst (2).
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{integral72_f5.ps} \end{figure}$	Figure 5: Average photon spectrum of X1901+03 measured with JEM-X and IBIS/ISGRI over the entire set of observations. Solid line shows the approximation by a power law with the high energy cutoff.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{integral72_f6.ps} \end{figure}$	Figure 6: The pulse profile of X1901+03 in the 5-15 keV energy band.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{integral72_f7.ps} \end{figure}$	Figure 7: Average photon spectra of XTE J1908+094, X1908+075 and 4U1907+097 obtained with the ISGRI instrument. Solid lines show the power law approximations.
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