All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig1.eps}\end{figure}$ Figure 1: In some cases the coordinates are not sufficient to identify a galaxy. This shows that often additional information is required. For instance for the pair of galaxies NGC 3314A and NGC 3314B.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig2.eps}\end{figure}$ Figure 2: In some cases the definition of what is a galaxy is difficult. The object ESO 267-41 = PGC 40012 is considered as three galaxies in the MCG catalog (MCG-7-26-1 MCG-7-26-2 and MCG-7-26-3).
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{ms3772_fig3.eps}\end{figure}$ Figure 3: Comparison of coordinates in LEDA with coordinates from SIMBAD (CDS).
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{ms3772_fig4.eps}\end{figure}$ Figure 4: Illustration of the EPIDEMIC method. The best and largest sample (here STD1) is used to convert the second best and largest sample STD2 to its scale. So, one obtains the new standard STD1+STD2. The process is applied to the next sample to get the next standard STD1+STD2+STD3, etc. In the present illustration, one can see that it would have been impossible to convert the sample STD4 to STD1 without the EPIDEMIC method.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig5.eps}\end{figure}$ Figure 5: Standard deviation of position angle as a function of $\log R_{25}$ . The solid curve give the adopted representation (Eq. (5)).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig6.eps}\end{figure}$ Figure 6: The identification of NGC 3314A and NGC 3314B can be made unambiguously using coordinates, diameter, axis ratio and position angle. Such an identification works even in the most difficult cases.
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In the text

$\begin{figure} \par\includegraphics[width=17.5cm,clip]{ms3772_fig7.eps}\end{figure}$ Figure 7: The equal-area galaxy distribution of the present catalog in supergalactic coordinates. The longitude $0^\circ$ is on the right, $360^\circ$ is on the left. Different regions can be identified: 1 = Pavo-Indus, 2 = Perseus-Pisces, 3 = Fornax, 4 = SMC, 5 = LMC, 6 = Centaurus, 7 = Virgo, 8 = Shapley concentration, 9 = Position of the putative Great Attractor. A part of the galactic plane is visible as a vertical lane with a few galaxies. The limit of the surveys in this zone of avoidance are clearly delimited.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig1.eps}\end{figure}$	Figure 1: In some cases the coordinates are not sufficient to identify a galaxy. This shows that often additional information is required. For instance for the pair of galaxies NGC 3314A and NGC 3314B.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig2.eps}\end{figure}$	Figure 2: In some cases the definition of what is a galaxy is difficult. The object ESO 267-41 = PGC 40012 is considered as three galaxies in the MCG catalog (MCG-7-26-1 MCG-7-26-2 and MCG-7-26-3).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{ms3772_fig3.eps}\end{figure}$	Figure 3: Comparison of coordinates in LEDA with coordinates from SIMBAD (CDS).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig5.eps}\end{figure}$	Figure 5: Standard deviation of position angle as a function of $\log R_{25}$ . The solid curve give the adopted representation (Eq. (5)).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{ms3772_fig6.eps}\end{figure}$	Figure 6: The identification of NGC 3314A and NGC 3314B can be made unambiguously using coordinates, diameter, axis ratio and position angle. Such an identification works even in the most difficult cases.
Open with DEXTER