\begin{table}%t6
%\centering
\par
\caption{\label{morphological_table}Morphological and environmental properties of 47 ADF-S galaxies used for fitting SED models.}
\begin{tabular}{cllc} 
\hline\hline \noalign{\smallskip}
ID  &  Type of source$^{{\rm a}}$ & Morphological type$^{{\rm b}}$ & Number of  \\
(ADFS)  &&  & counterparts$^{{\rm c}}$\\
\hline
1 & Galaxy/IRS/RS  & Sb  & 1 \\  
2 & Galaxy in Pair of Interacting Galaxies/IRS/RS  & E  & 1 \\  
3 & Galaxy/IRS/RS/other  & Sa  & 1 \\  
4 & Stardust Galaxy IR emission line up with  & S0, SA0- pec: HII  BCDG  & 1\\   & Super Star Cluster/IRS/RS/other  & &\\
5 & Galaxy/IRS/RS  & S  & 2 \\  
6 & Galaxy/IRS  & --  & 4 \\  
7 & Galaxy in Cluster of Galaxies/IRS  & S0\tablefootmark{1}  & 1\\  
8 & Galaxy in Cluster of Galaxies/IRS  & Sb\tablefootmark{1}  & 2\\  
9 & Galaxy in Cluster of Galaxies  & Sb\tablefootmark{1} & 3\\  
10 & Galaxy in Cluster of Galaxies/IRS/RS  & S00 pec\tablefootmark{1} & 1\\  
11 & Galaxy in Cluster of Galaxies/IRS/RS  & SB\tablefootmark{1} & 1\\  
12 & IRS & --  & 1\\  
13 & Galaxy/IRS  & --  & 2\\  
14 & Galaxy/IRS/RS  & --  & 2\\  
15 & Galaxy/IRS  & --  & 3\\  
16 & IRS/Galaxy in Pair of Galaxies  & --  & 2\\  
17 & Interacting Galaxies/IR/RS  & Sbc pec & 3\\  
18 & Galaxy/IRS  & S  & 1\\  
19 & Galaxy/IRS  & --  &  2\\  
20 & Galaxy/IRS  & --  & 1\\  
21 & Galaxy/IRS  & SAB  & 1\\  
22 & Galaxy/IRS  & S  & 2\\  
23 & Interacting Galaxies& cG (compact G), Chain of 3 galaxies& 1\\
24 & Galaxy/IRS  & S  & 2\\  
26 & Galaxy  & --  & 2\\  
27 & IRS  & --  & 1\\  
29 & Galaxy/IRS  & S0a  & 1\\  
30 & IRS/Galaxy  & --  & 1\\  
31 & IRS/Galaxy  & --  & 1\\  
39 & Galaxy/IRS  & S0  & 3\\  
41 & Galaxy/IRS  & --  & 2\\  
42 & Galaxy/IRS  & --  & 1\\  
43 & IRS/Galaxy  & --  & 1\\  
45 & Galaxy in Cluster of Galaxies/IRS  & Sbp\tablefootmark{1} & 1\\  
46 & Galaxy/IRS  & --  & 1\\  
48 & Galaxy/IRS  & --  & 1\\  
49 & Galaxy  & --  & 2\\  
50 & Galaxy/IRS  & S  & 1\\  
51 & Galaxy/IRS/RS  & SB & 1\\  
52 & IRS/Galaxy  & --  & 1\\  
56 & Galaxy/IRS  & --  & 5\\  
64 & Galaxy/IRS  & Sc  & 1\\  
65 & Galaxy in Cluster of Galaxies/IRS  &  S0\tablefootmark{1} & 1\\  
69 & Galaxy/ IRS  & --  & 2\\  
72 & Galaxy in Cluster of Galaxies/IRS  & Sbb pec\tablefootmark{1}  & 2\\  
73 & IRS  & --  & 1\\  
82 & Galaxy  & --  & 1\\  
103 & Galaxy in Cluster of Galaxies/IRS  &  Sb\tablefootmark{1}& 2\\  
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{The object classification: Galaxy means that it has been identified as a galaxy, IRS means that it has been previously identified as the infra-red source, RS means that it has been identified as the radio source, ``other'' means that it has been observed in some other (UV or X-ray) wavelengths. This column contains also the available information about the object's environment - whether it is an object from the cluster  of galaxies (in this case it always applies to Abell~S0463) or an interacting group of galaxies.} 
\tablefoottext{b}{The object's indicative morphological type, as provided by the NED.} 
\tablefoottext{c}{The number of counterparts found for each object in our 40'' search range, which may be treated as a very crude indicator of the local environment of an investigated object.}
\tablefoottext{1}{\cite{dressler80a}.}}
\end{table}