All Figures

$\begin{figure} \par\mbox{\epsfig{file=im_a1.ps,width=8cm} } \end{figure}$ Figure 1: Surface brightness images for NGC 3344, J and $K_{\rm s}$ (top panels, left to right) and NGC 3686, J and $K_{\rm s}$ (bottom panels, left to right).
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In the text

$\begin{figure} \par\mbox{\epsfig{file=im_a2.ps,width=8cm} } \end{figure}$ Figure 2: Surface brightness images for NGC 3938, J and $K_{\rm s}$ (top panels, left to right) and NGC 3953, J and $K_{\rm s}$ (bottom panels, left to right).
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In the text

$\begin{figure} \par\mbox{\epsfig{file=im_a3.ps,width=8cm} } \end{figure}$ Figure 3: Surface brightness images for NGC 4254, J and $K_{\rm s}$ (top panels, left to right) and NGC 4303, J and $K_{\rm s}$ (bottom panels, left to right).
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In the text

$\begin{figure} \par\mbox{\epsfig{file=im_a4.ps,width=8cm} } \end{figure}$ Figure 4: Surface brightness images for NGC 4314, J and $K_{\rm s}$ (top panels, left to right) and NGC 5248, J and $K_{\rm s}$ (bottom panels, left to right).
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In the text

$\begin{figure} \par\mbox{\epsfig{file=im_a5.ps,width=8cm} } \end{figure}$ Figure 5: Surface brightness images for NGC 6384, J and K (top panels, left to right) and NGC 7479, J and $K_{\rm s}$ (bottom panels, left to right).
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In the text

$\begin{figure} \par\mbox{\epsfig{file=comparacion_f.ps,width=8.8cm} } \end{figure}$ Figure 6: Correlation between the two sets of parameters for the brightness profiles: isophotal parameters (i) vs. fitting parameters (f). The graphic represents the ratio between the same parameters of each galaxy's surface brightness decomposition calculated using the two methods. See caption of Table 5 for an explanation of the parameter names in the x-axis.
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In the text

$\begin{figure} \par\mbox{\epsfig{file=im_a1.ps,width=8cm} } \end{figure}$	Figure 1: Surface brightness images for NGC 3344, J and $K_{\rm s}$ (top panels, left to right) and NGC 3686, J and $K_{\rm s}$ (bottom panels, left to right).
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=im_a2.ps,width=8cm} } \end{figure}$	Figure 2: Surface brightness images for NGC 3938, J and $K_{\rm s}$ (top panels, left to right) and NGC 3953, J and $K_{\rm s}$ (bottom panels, left to right).
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=im_a3.ps,width=8cm} } \end{figure}$	Figure 3: Surface brightness images for NGC 4254, J and $K_{\rm s}$ (top panels, left to right) and NGC 4303, J and $K_{\rm s}$ (bottom panels, left to right).
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=im_a4.ps,width=8cm} } \end{figure}$	Figure 4: Surface brightness images for NGC 4314, J and $K_{\rm s}$ (top panels, left to right) and NGC 5248, J and $K_{\rm s}$ (bottom panels, left to right).
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=im_a5.ps,width=8cm} } \end{figure}$	Figure 5: Surface brightness images for NGC 6384, J and K (top panels, left to right) and NGC 7479, J and $K_{\rm s}$ (bottom panels, left to right).
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=comparacion_f.ps,width=8.8cm} } \end{figure}$	Figure 6: Correlation between the two sets of parameters for the brightness profiles: isophotal parameters (i) vs. fitting parameters (f). The graphic represents the ratio between the same parameters of each galaxy's surface brightness decomposition calculated using the two methods. See caption of Table 5 for an explanation of the parameter names in the x-axis.
Open with DEXTER