\begin{table}%t3
\caption{\label{datos}Integral field spectroscopy observations log. The galaxies are sorted by decreasing nuclear distance.}   
\small%\centerline
{  
\begin{tabular}{lccccc} 
\hline 
\hline
\noalign{\smallskip}
IRAS Name & INTEGRAL & INTEGRAL & Date & Exp. time & Comment on IFU data\\
 & (Bundle) & (FoV arcsec$^{2}$) &month/year & (s) & \\
\hline
IRAS~13156+0435  & SB2, SB3 & 32.9~$\times$~25.3, 69.1~$\times$~60.5& 03/02 & 17~400$^a$  & [O~{\sc iii}] non detected in N comp. \\
IRAS~13342+3932  & SB3   & 101.7~$\times$~89.0& 03/02 & 6~$\times$~1500     &                   \\
IRAS~18580+6527   & SB2   & 47.8~$\times$~36.7 & 04/01 & 7~$\times$~1500     &                    \\
IRAS~16007+3743$^{b}$   & SB2   & 49.6~$\times$~38.1 & 04/01 & 6~$\times$~1500     &                    \\
IRAS~06268+3509 & SB2  & 46.3~$\times$~35.6 & 03/02 & 6~$\times$~1500      &                   \\
IRAS~08572+3915$^b$  & SB2   & 18.0~$\times$~13.9 & 04/99 & 9~$\times$~1800      &                    \\
IRAS~14348$-$1447$^{a}$ & SB2   & 1.3~$\times$~1.0& 04/98 & 4~$\times$~1800     &                    \\ 
Arp~299$^c$  & SB2, SB3 & 3.3~$\times$~2.5, 6.9~$\times$~6.0& 01/04 & 12~600$^d$  & \\
IRAS~13469+5833  & SB1   & 21.3~$\times$~17.4& 03/02 & 5~$\times$~1800     & Sky line to H$\alpha$+[N~{\sc ii}] complex\\
         &     & &    &            & Not enough S/N                        \\
IRAS~12112+0305$^{a}$~$^e$  & SB2   & 27.9~$\times$~19.5& 04/98 & 5~$\times$~1800, 4~$\times$~1500    & \\
Mrk~463      & SB2   & 15.7~$\times$~12.1& 04/01 & 5~$\times$~900      &                    \\
IRAS~06487+2208  & SB1   & 19.7~$\times$~16.1 & 03/02 & 5~$\times$~1500      &                    \\
IRAS~11087+5351  & SB1   & 19.5~$\times$~16.0& 03/02 & 6~$\times$~1500     &                    \\
Mrk~273$^{a}$      & SB2   & 12.0~$\times$~9.2& 04/98 & 3~$\times$~1500     &                    \\
Arp~220$^{a}$ & SB2, SB3 & 5.9~$\times$~4.5, 12.4~$\times$~10.8 & 05/00 & 48~000$^f$ & [O~{\sc iii}] not detected, H$\beta$ not covered \\	
IRAS~17208$-$0014$^{a}$ & SB2   & 13.5~$\times$~10.4 & 04/99 & 4~$\times$~1950     &                    \\
IRAS~15250+3609$^{a}$  & SB2   & 17.1~$\times$~13.2& 04/98 & 5~$\times$~1800     &                    \\
IRAS~12490$-$1009 & SB2   & 29.7~$\times$~22.8& 03/02 & 4~$\times$~1500     &                    \\
IRAS~14060+2919  & SB2   & 1.9~$\times$~1.4& 03/02 & 4~$\times$~1800     &                    \\ 
IRAS~09427+1929  & SB3   & 87.4~$\times$~76.4 & 03/02 & 2320$^g$ & Short inhomogeneous exposures\\
IRAS~15206+3342$^{a}$   & SB2   & 35.7~$\times$~27.4& 04/99 & 4~$\times$~1800     &                    \\ 
Mrk~231      & SB1   & 6.5~$\times$~5.3& 03/02 & 4~$\times$~900      & H$\beta$ not covered         \\ 
         &     & &    &            & Broad emission lines          \\
\hline                                  
\end{tabular}}\label{Table_log}
\smallskip
 $^a$ {3~$\times$~1500 s for the South component with the SB2 bundle; 3~$\times$~1800 for the North component with the SB2 bundle, 5~$\times$~1500 s for the entire system with the SB3 bundle.}\\
  $^b$  {Previously published galaxy. See Colina et~al. (\cite{Colina2005}), Monreal-Ibero et~al. (\cite{Monreal2007}) and references therein.}\\
   $^c$ {Garc\'{\i}a-Mar\'{\i}n et~al. (\cite{Garc2006}).}\\
 $^d$ {3~$\times$~1200 s for each individual galaxy of the system, NGC~3690 and IC~694 observed with the SB2 bundle. 3~$\times$~1800 s for the entire system as observed with the SB3 bundle.}\\
 $^e$ {For IRAS~12112+0305 we present the results obtained by combining two different pointings of the SB2 INTEGRAL bundle.}\\
 $^f$ {6~$\times$~1500 s for the nuclear region observed with the SB2 bundle, 26~$\times$~1500 s for the nucleus and the extended nebula as observed with the SB3~bundle.}\\
 $^g$ {1500 s, 520 s, 300 s.} 
\end{table}