\begin{table}%t1
\caption{\label{Tab1}Log of the PMAS observations.}
%\centerline
 {\small \begin{tabular}{lcccccccc}
\hline\hline\noalign{\smallskip}
Galaxy  & Dist & $\log L_{\rm IR}$ & Date  &  Galaxy $t_{\rm int}$ &      Sky $t_{\rm int}$  & Airmass & Seeing & Conditions\\  
(1)     & (2) & (3)  & (4) & (5) & (6) & (7) & (8) & (9)\\
\hline
NGC~23  &  59.6 & 11.05 & 7 Nov. 2005 & $3 \times 1000$
&  1000  & 1.06& $1.0{-}1.2$ & P\\ 
MCG~+12-02-001 & 64.3 & 11.44 & 18 Dec. 2006 & $4 \times 800$ &
1000 &  1.47 &1.7 & NP\\ 
UGC~1845 & 62.0 & 11.07 & 8 Nov. 2005 & $3 \times 900$  &900   &  1.05& $1.4{-}2.0$ & NP\\ 
NGC~2388   & 57.8 & 11.23: & 7 Nov. 2005 & $3 \times 1000$ & 1000  &  1.04& $1.3{-}1.1$ & P\\ 
MCG~+02-20-003 & 67.6 & 11.08: & 17 Dec. 2006 & $4\times 800$  & 1000
 &  1.60 & 1.2 & NP\\ 
IC~860 & 59.1 & 11.17: & 30 May 2006 & $4\times 800$ & 1000 &  1.03& 1.7 & NP\\ 
NGC~5936&60.8& 11.07& 30 May 2006 & $4\times 800$ &1000 & 1.17& 1.5 & NP\\ 
NGC~6701  &  56.6 & 11.05 &  30 May 2006 & $1\times400 +
4\times 600$   &  800 &1.09 &1.3 & NP\\ 
NGC~7469 &  65.2 & 11.59 & 8~Nov. 2005 & $3 \times 900$ &900 &1.15& 1.2 & NP\\ 
NGC~7591 &65.5 & 11.05 & 8 Nov. 2005 & $3 \times 1000$ & 1000 & 1.32& $1.1{-}1.2$ & NP\\ 
NGC~7771-E & 57.1 & 11.34 & 7 Nov. 2005  & $2\times 500 +
2\times 1000$ & 1000 & 1.15 & 0.8 & P\\ 
NGC~7771-W    & $\cdots$  &$\cdots$  & 7 Nov. 2005   & $3 \times 1000$  &
1000 &   1.06  & 0.8 & P\\ 
\hline 
\end{tabular} }
\medskip
Notes. -- Column~(1): galaxy. For NGC~7771 we took two different pointings to cover the approximate central $28 \arcsec \times 16 \arcsec$ region of the galaxy, as explained in the text. Columns~(2) and (3): distance (in Mpc) and IR luminosity (in $L_\odot$) taken from Sanders et~al. (\cite{sanders2003}) for the {IRAS}~RBGS. Column~(4): date of the observations. Column~(5): integration time (in seconds) of the galaxy observations after discarding bad data sets. Column~(6): integration time (in seconds) of the sky observations. Column~(7):  airmass at the beginning of the observation. Column~(8): typical seeing  conditions (in arcseconds) of the observations.  If two values of the seeing are given they  correspond to the beginning and the end of the observations. Column~(9): observing conditions. P:~Photometric. NP:~Non-photometric.
\end{table}