\begin{table}%t3
\par
\caption {\label{tab:param}Physical parameters derived from the SED analysis and from the HR diagram. 
} 
%\centerline
 \begin{tabular}{ l l l l l l l l r c c c} % left columns (10 columns)
\hline\hline 
  Id  &   2MASS		    & Other  & $T_{\rm eff}$ &  $L$           & $A_V$	  & $R$      & $M$	      &  Age  & \multicolumn{3}{c}{Membership} \\
      &                     & Id &  (K)          &  ($L_{\odot}$)  & (mag)	  & ($R_{\odot}$) & ($M_{\odot}$)   &  (Myr)  & Ph$^{{a}}$ 
      & Sp$^{{b}}$ & As$^{{c}}$ \\ 
\hline 
  ~1  &  {\scriptsize 05352184-0546085}   &                   &  2700	   &   0.036 &	1.10  &   0.87 &     0.04 & $\leq$1 &  Y &  ... &  ...	\\ 
{\it ~2}&  {\scriptsize 05352029-0546399} &                   & {\it 3710} &   0.260 &	0.20  &   1.24 &     0.70 &	7.1  &  Y &  Y   &  ...	\\ 
   ~3  &  {\scriptsize 05352021-0546510}  &                   &  3800	   &   0.436 &	0.13  &   1.52 &     0.85 &	5.1  &  Y &  ... &  Y	\\ 
{\it ~4}&  {\scriptsize 05352007-0545526} &\object{Parenago 1980}& {\it 5720}& 0.581 &	2.55  &   ...  &     ...  &	...  &  N &  N   &  ...	\\ 
   ~5  &  {\scriptsize 05351981-0545409}  & \object{V1732 Ori}&  3400	   &   0.213 &	0.07  &   1.33 &     0.40 &	2.8  &  Y &  ... &  Y	\\ 
   ~6  &  {\scriptsize 05351903-0546163}  &        	      &  3700	   &   0.303 &  0.12  &   1.34 &     0.62 &	4.0  &  Y &  ... &  ... \\ 
   ~7  &  {\scriptsize 05351924-0547012}  &        	      &  3300	   &   0.122 &  0.88  &   1.07 &     0.25 &	2.5  &  Y &  Y   &  ... \\ 
   ~8  &  {\scriptsize 05351950-0547457}  &        	      &  3800	   &   0.188 &  0.19  &   1.00 &     0.80 &    20.1  &  P &  ... &  ... \\ 
{\it ~9}&  {\scriptsize 05352281-0544428} & \object{V1529 Ori}& {\it 3480} &   0.658 &	0.89  &   1.98 &     0.70 &	1.6  &  Y &  Y   &  ...	\\ 
{\it 10}&  {\scriptsize 05352617-0545084} &                   & {\it 4110} &   0.403 &	1.06  &   1.25 &     1.00 &    10.0  &  Y &  Y   &  ...	\\	   
  11  &  {\scriptsize 05352550-0545448}   & \object{NR Ori}   &  3800	   &   0.261 &	0.56  &   1.18 &     0.80 &    10.0  &  Y &  ... &  ...	\\ 
  12  &  {\scriptsize 05351695-0545558}   &         	      &  3200	   &   0.354 &  0.70  &   1.94 &     0.30 &	1.0  &  Y &  Y   &  ... \\ 
{\it 13}&  {\scriptsize 05351621-0547201} &         	      & {\it 5800} &   0.887 &  2.72  &   ...  &     ...  &    ...   &  N &  N   &  ... \\ 
{\it 14}&  {\scriptsize 05351192-0545379} & \object{V1490 Ori}& {\it 4250} &   1.046 &	1.21  &   1.89 &     1.30 &	4.0  &  Y &  Y   &  Y	\\ 
  15  &  {\scriptsize 05351290-0545376}   &                   &  3500	   &   0.170 &  1.42  &   1.12 &     0.40 &	4.0  &  Y &  Y   &  ... \\ 
  16  &  {\scriptsize 05351797-0549375}   & \object{V793 Ori} &  4000	   &   0.506 &  0.17  &   1.48 &     1.00 &	6.4  &  Y &  ... &  ... \\ 
  17  &  {\scriptsize 05350614-0545311}   & \object{V482 Ori} &  4400	   &   0.531 &  0.28  &   1.26 &     1.10 &    16.0  &  P &  ... &  Y	\\ 
  18  &  {\scriptsize 05353222-0544265}   &\object{Parenago 2103} &  3600  &   0.700 &  0.11  &   2.16 &     0.62 &	1.0  &  Y &  ... &  Y	\\ 
  19  &  {\scriptsize 05352973-0548450}   & \object{V498 Ori} &  4400	   &   1.763 &  0.37  &   2.29 &     1.40 &	5.0  &  Y &  ... &  ... \\ 
  20  &  {\scriptsize 05350738-0548010}   &                   &  2900	   &   0.321 &  0.67  &   2.25 &      ... &     ...  &  P &  Y   &  ... \\ 
{\it 21}&  {\scriptsize 05351033-0546335} & \object{AA Ori}   & {\it 4830} &  12.39  &	2.50  &   4.72 &     2.7  & $\leq$$ 1$ &  Y &  Y   &  Y	\\ 
  22  &  {\scriptsize 05351205-0547296}   &         	      &  2800	   &   0.061 &  0.35  &   1.05 &     0.06 & $\leq $$1$ &  Y &  ... &  ... \\ 
{\it 23}&  {\scriptsize 05351011-0548342} &         	      & {\it 3690} &   0.117 &  0.10  &   0.84 &     0.62 &    18.0  &  P &  Y   &  ... \\ 
  25  &  {\scriptsize 05351493-0549348}   &         	      &  5000	   &   0.633 &  0.17  &   1.06 &     0.95 &    40.0  &  N &  ... &  ... \\ 
  27  &  {\scriptsize 05352637-0544340}   &         	      &  3600	   &   0.071 &  0.07  &   0.69 &     0.60 &    28.0  &  P &  Y   &  ... \\ 
{\it 28}&  {\scriptsize 05351423-0543175} & \object{AB Ori}   & {\it 4260} &   4.812 &	1.88  &   3.28 &     1.7  &	9.0  &  Y &  Y   &  Y	\\ 
  29  &  {\scriptsize 05351236-0543184}   & \object{V486 Ori} &  4400	   &   1.174 &	0.21  &   1.87 &     1.40 &	5.0  &  Y &  ... &  Y	\\ 
  30  &  {\scriptsize 05351146-0544183}   &         	      &  3200	   &   0.083 &  0.52  &   0.94 &     0.18 &	2.3  &  Y &  Y   &  ... \\ 
  31  &  {\scriptsize 05350575-0544001}   &         	      &  3800	   &   0.210 &  0.22  &   1.06 &     0.70 &    10.1  &  P &  ... &  ... \\ 
  32  &  {\scriptsize 05350567-0543046}   &         	      &  3200	   &   0.050 &  0.01  &   0.73 &     0.18 &	4.5  &  Y &  ... &  ... \\ 
33$^*$ & {\scriptsize 05350486-0544267}   &         	      &  4600	   &   0.095 &  3.58: &   0.49 &     ...  &	...  &  N &  ... &  ... \\ 
  35  & {\scriptsize 05350303-0545333}    &         	      &  4600	   &   0.896 &  4.75  &   1.49 &     1.20 &    16.0  &  P &  Y   &  ... \\
  39  &  {\scriptsize 05350406-0548540}   &         	      &  3800	   &   0.121 &  0.06  &   0.80 &     0.70 &    28.2  &  P &  Y   &  ... \\ 
40$^*$ &  {\scriptsize 05350627-0549021}  &         	      &  2000	   &   0.196 &  4.18: &   3.69 &     ...  &	...  &  P &  ... &  ... \\ 
  41  &  {\scriptsize 05350825-0550003}   &         	      &  3900	   &   0.204 &  0.02  &   0.99 &     0.80 &    15.9  &  P &  ... &  ... \\ 
  42  &  {\scriptsize 05351088-0549485}   &         	      &  3400	   &   0.057 &  0.01  &   0.69 &     0.40 &    20.1  &  P &  ... &  ... \\ 
  47  &  {\scriptsize 05353023-0551169}   &         	      &  4400	   &   0.489 &  0.14  &   1.21 &     1.05 &    20.0  &  P &  ... &  ... \\  
{\it 48}&  {\scriptsize 05353047-0549037} &         	      & {\it 3830} &   0.208 &  0.10  &   1.04 &     0.75 &    12.5  &  P &  Y   &  Y	\\ 
  49  &  {\scriptsize 05353294-0549326}   &         	      &  3700	   &   0.042 &  0.05  &   0.50 &     0.50 &    71.3  &  N &  ... &  ... \\ 
  50  &  {\scriptsize 05353385-0548211}   &         	      &  3300	   &   0.069 &  0.91  &   0.80 &     0.25 &	5.6  &  Y &  ... &  ... \\ 
{\it 51}&  {\scriptsize 05353316-0547074} & \object{V1744 Ori}& {\it 3690} &   0.140 &	0.10  &   0.92 &     0.57 &    11.3  &  P &  Y   &  ...	\\	    
{\it 52}&  {\scriptsize 05352930-0545381} & \object{V1551 Ori}& {\it 3740} &   0.185 &	0.03  &   1.03 &     0.62 &	8.9  &  Y &  Y   &  ...	\\ 
  53  &  {\scriptsize 05353372-0546162}   &          	      &  3800	   &   0.124 &  0.06  &   0.81 &     0.70 &    25.4  &  P &  ... &  ... \\ 
  54  &  {\scriptsize 05353266-0545284}   &          	      &  3100	   &   0.041 &  0.05: &   0.70 &     0.10 &	2.5  &  Y &  Y   &  ... \\ 
  55  &  {\scriptsize 05353229-0544060}   & \object{V1564 Ori}&  3800	   &   0.145 &	0.22  &   0.88 &     0.75 &    28.2  &  P &  ... &  ...	\\ 
{\it 56}&  {\scriptsize 05353092-0543053} & \object{V1556 Ori}& {\it 3920} &   0.874 &	0.05  &   1.38 &     0.90 &	6.4  &  Y &  Y   &  Y	\\ 
  57  &  {\scriptsize 05352765-0542551}   &\object{Parenago 2059}& 4200	   &   0.816 &	1.69  &   1.71 &     1.20 &	5.0  &  Y &  ... &  Y   \\ 
  58  &  {\scriptsize 05352634-0543364}   &                   &  2900	   &   0.051 &  0.23  &   0.89 &     0.08 &	1.0  &  Y &  ... &  ... \\ 
  59  &  {\scriptsize 05352125-0542123}   & \object{V416 Ori} &  3700	   &   0.343 &  0.01  &   1.43 &     0.70 &	4.5  &  Y &  Y   &  Y	\\ 
  60  &  {\scriptsize 05351643-0542396}   & \object{V1506 Ori}&  4800	   &   0.934 &  0.03  &   1.40 &     1.15 &    20.0  &  P &  ... &  Y	\\ 
  61  &  {\scriptsize 05351734-0542145}   & \object{V411 Ori} &  3800	   &   0.356 &  0.73  &   1.38 &     0.75 &	5.0  &  Y &  Y   &  ... \\ 
  62  &  {\scriptsize 05351715-0541538}   & \object{V1507 Ori}&  3300	   &   0.149 &  0.41  &   1.18 &     0.35 &	3.6  &  Y &  ... &  ... \\ 
  63  &  {\scriptsize 05351123-0541361}   & \object{V1489 Ori}&  3600	   &   0.210 &  2.65  &   1.18 &     0.50 &	4.5  &  Y &  ... &  ... \\ 
{\it 65}&  {\scriptsize 05345908-0544303} & \object{KT Ori}   & {\it 3990} &   0.975 &	0.48  &   2.07 &     1.10 &	2.5  &  Y &  Y   &  ...	\\  
66$^*$  &  {\scriptsize 05345923-0544553} &	    	      &  4600	   &   1.210 &  4.96: &   1.74 &     1.40 &	9.0  &  Y &  ... &  ... \\  
69$^*$  &  {\scriptsize 05345898-0547596} &	    	      &  2900	   &   0.897 &  3.47  &   3.76 &     ...  &    ...   &  P &  ... &  ... \\  
{\it 70}&  {\scriptsize 05350054-0548591} &         	      & {\it 4600} &   0.904 &  4.07  &   1.50 &     1.20 &    16.0  &  P &  Y   &  ... \\  
75  &  {\scriptsize 05350284-0551031}   &         	     	 &  4800     &   0.447 &   1.75  &   0.97 &	0.90 &    39.8  &  N &  ... &  ... \\  
  80  &  {\scriptsize 05353168-0542457}   &         	     	 &  3800     &   0.091 &   0.29  &   0.70 &	0.62 &    40.2  &  N &  ... &  ... \\ 
  86  &  {\scriptsize 05351895-0545117}   &         	     	 &  3900     &   0.032 &   0.03  &   0.39 &	...  &     ...  &  N &  ... &  ... \\ 
\hline
    89  &  {\scriptsize 05353692-0543172}   &         	     	 &  3400     &   0.042 &   0.09  &   0.59 &	0.25 &    11.3  &  P &  ... &  ... \\ 
  90  &  {\scriptsize 05352650-0548497}   &\object{Parenago 2049}&  3800     &   0.488 &   0.00  &   1.61 &	0.85 &     4.0  &  Y &  ... &  ... \\ 
  91  &  {\scriptsize 05352707-0548522}   &\object{Parenago 2050}&  3800     &   0.945 &   0.00  &   2.25 &	0.85 &     1.3  &  Y &  ... &  ... \\ 
  92  &  {\scriptsize 05351197-0541521}   &	            	 &  3800     &   0.041 &   0.25  &   0.47 &     ...  &     ...  &  N &  ... &  ... \\ 
{\it  93} & {\scriptsize 05351790-0542340}&\object{Parenago 1929}&{\it 4775} &   4.792 &   0.58  &   3.20 &     1.8  &     1.0  &  Y &  ... &  ... \\ 
  94  &  {\scriptsize 05352080-0544527}   &                 	 &  4200     &   0.025 &   0.52  &   0.30 &     ...  &     ...  &  N &  ... &  ... \\ 
\hline
\end{tabular}                	                 
\par
\smallskip    	                 
 $^{{a}}$  Photometric membership (present work). 
 $^{{b}}$  Spectroscopic membership based on the radial velocity and/or H$\alpha$~emission \citep{Furesz08}.
 $^{{c}}$~Astrometric membership based on proper motions \citep{Dias06}.
 $^*$  Unreliable parameters due to the lack of optical photometry and a likely strong reddening and/or NIR~excess.\\
 Effective temperatures constrained from spectroscopy are indicated in italics.	         	                	           
 \end{table}