$\begin{figure} \par\includegraphics[angle=270,width=9cm,clip]{8774abs.ps}\end{figure}$ Figure 1: Adopted extinction law. We used the law given in Cardelli et al. (1989) in the optical, the one given in Indebetouw et al. (2005) from 1.25 $\mu {{\rm m}}$ to 8 $\mu {{\rm m}}$ , and the law from Lutz et al. (1996) above 8 $\mu {{\rm m}}$ .
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In the text

$\begin{figure} \par\includegraphics[width=4.7cm,clip]{8774140p.eps}\end{figure}$ Figure 2: VISIR image of IGR J19140+0951 in PAH1 (8.59 $\mu$ m). 19 $.\!\!^{\prime\prime}$ 2 $\times$ 19 $.\!\!^{\prime\prime}$ 2 field of view and 0 $.\!\!^{\prime\prime}$ 075 plate scale. We clearly see the two sources that were blended with MSX. The MIR counterpart of IGR J19140+0951 is the northern source.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{8774195d.eps}\par\includegra... ...lip]{8774318d.eps}\par\includegraphics[width=8cm,clip]{8774358d.eps}\end{figure}$ Figure 4: IR SEDs of IGR J16195-4945, IGR J16318-4848, and IGR J16358-4726 in the NIR and the MIR. We show their SEDs including the contribution of the star and the dust (line), the star only (dashed-line), and the dust only (dotted-line).
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=9cm,clip]{8774abs.ps}\end{figure}$	Figure 1: Adopted extinction law. We used the law given in Cardelli et al. (1989) in the optical, the one given in Indebetouw et al. (2005) from 1.25 $\mu {{\rm m}}$ to 8 $\mu {{\rm m}}$ , and the law from Lutz et al. (1996) above 8 $\mu {{\rm m}}$ .
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$\begin{figure} \par\includegraphics[width=4.7cm,clip]{8774140p.eps}\end{figure}$	Figure 2: VISIR image of IGR J19140+0951 in PAH1 (8.59 $\mu$ m). 19 $.\!\!^{\prime\prime}$ 2 $\times$ 19 $.\!\!^{\prime\prime}$ 2 field of view and 0 $.\!\!^{\prime\prime}$ 075 plate scale. We clearly see the two sources that were blended with MSX. The MIR counterpart of IGR J19140+0951 is the northern source.
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$\begin{figure} \par\mbox{\includegraphics[angle=-90,width=5.5cm,clip]{8774195.ep... ...e*{3mm} \includegraphics[angle=-90,width=5.5cm,clip]{8774140.eps} } \end{figure}$	Figure 3: Optical-to-MIR absorbed (line) and unabsorbed (dotted-line) SEDs of 12 INTEGRAL sources, including broad-band photometric data from ESO/NTT, 2MASS, GLIMPSE, and VISIR.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{8774195d.eps}\par\includegra... ...lip]{8774318d.eps}\par\includegraphics[width=8cm,clip]{8774358d.eps}\end{figure}$	Figure 4: IR SEDs of IGR J16195-4945, IGR J16318-4848, and IGR J16358-4726 in the NIR and the MIR. We show their SEDs including the contribution of the star and the dust (line), the star only (dashed-line), and the dust only (dotted-line).
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