\begin{table}{}%tD.2
\scriptsize
%\centering
\par
\caption{Photometric data.}
\label{photodata}
\begin{tabular}{lrrc|lrrc|lrrc}
\hline\hline\noalign{\smallskip}
Star & $\lambda$ & $F_{\nu}$ & Reference & Star & $\lambda$ & $F_{\nu}$ & Reference & Star & $\lambda$ & $F_{\nu}$ & Reference \\
\hline
  & [$\mu$m] & [Jy] &  &   & [$\mu$m] & [Jy] &  &   & [$\mu$m] & [Jy] &  \\
\hline 
$o$~Cet 	&	0.55	&	229.94	&	(1)	&	CW~Leo	&	1.25	&	2.3	&	(21)	&	WX~Psc	&	1.23	&	3.17	&	(1)	\\
	&	0.55	&	9.76	&	(9)	&		&	1.25	&	2.7	&	(2)	&		&	1.25	&	1.69	&	(2)	\\
	&	0.7	&	1104.27	&	(10)	&		&	1.65	&	74.9	&	(2)	&		&	1.65	&	14.25	&	(2)	\\
	&	0.7	&	1138.92	&	(1)	&		&	1.65	&	39.6	&	(21)	&		&	2.17	&	86.52	&	(2)	\\
	&	0.88	&	2131.97	&	(1)	&		&	2.17	&	469	&	(2)	&		&	2.2	&	113.8	&	(1)	\\
	&	0.88	&	5871.93	&	(1)	&		&	2.2	&	388.8	&	(21)	&		&	3.5	&	220	&	(3)	\\
	&	0.9	&	5027.64	&	(10)	&		&	2.2	&	321.9	&	(3)	&		&	3.5	&	330.67	&	(1)	\\
	&	1.04	&	7193.59	&	(10)	&		&	3.5	&	3046.1	&	(3)	&		&	4.9	&	365.1	&	(3)	\\
	&	1.25	&	3128.15	&	(2)	&		&	3.6	&	9072	&	(21)	&		&	12	&	1120	&	(4)	\\
	&	1.25	&	9698.38	&	(10)	&		&	4.9	&	9010.7	&	(3)	&		&	12	&	646.9	&	(3)	\\
	&	1.25	&	3845.33	&	(1)	&		&	10.2	&	39188.4	&	(21)	&		&	25	&	929.3	&	(3)	\\
	&	1.25	&	9748.4	&	(1)	&		&	12	&	47500	&	(6)	&		&	25	&	921	&	(4)	\\
	&	1.65	&	4364.15	&	(2)	&		&	12	&	31773.4	&	(3)	&		&	34.6	&	498.5	&	(5)	\\
	&	2.17	&	5118.35	&	(2)	&		&	25	&	23100	&	(6)	&		&	60	&	212	&	(4)	\\
	&	2.2	&	11275.24	&	(1)	&		&	25	&	28610.8	&	(3)	&		&	60	&	175.3	&	(3)	\\
	&	2.2	&	5446.6	&	(1)	&		&	60	&	5650	&	(6)	&		&	100	&	68.8	&	(3)	\\
	&	2.2	&	5927.1	&	(3)	&		&	60	&	5585	&	(3)	&		&	100	&	67.5	&	(4)	\\
	&	2.25	&	11149.2	&	(10)	&		&	100	&	2017.5	&	(3)	&		&	400	&	3	&	(14)	\\
	&	3.5	&	4334.9	&	(3)	&		&	100	&	922	&	(6)	&		&	1200	&	0.16	&	(19)	\\
	&	3.5	&	10023.4	&	(10)	&		&	140	&	1051.5	&	(3)	&		&	1200	&	0.33	&	(19)	\\
	&	3.5	&	4606.73	&	(1)	&		&	377	&	35.2	&	(22)	&		&	1300	&	0.08	&	(13)	\\
																				\cline{9-12}									
	&	4.9	&	3220.5	&	(3)	&		&	400	&	32	&	(14)	&		&		&		&				\\
	&	5	&	5425.61	&	(1)	&		&	450	&	18.45	&	(12)	&	$\pi$~Gru	&	0.55	&	8.5	&	(1)	\\
	&	12	&	2415.6	&	(3)	&		&	450	&	29	&	(14)	&		&	0.55	&	10.22	&	(9)	\\
	&	12	&	4880	&	(6)	&		&	450	&	33.2	&	(16)	&		&	0.7	&	157.21	&	(1)	\\
	&	25	&	2322.8	&	(3)	&		&	800	&	6.66	&	(16)	&		&	0.88	&	1602.43	&	(1)	\\
	&	25	&	2260	&	(6)	&		&	811	&	9.8	&	(22)	&		&	1.25	&	3079.56	&	(2)	\\
	&	60	&	301	&	(6)	&		&	850	&	9.45	&	(12)	&		&	1.25	&	2943.97	&	(1)	\\
	&	60	&	263.2	&	(3)	&		&	900	&	9	&	(14)	&		&	1.65	&	5795.62	&	(2)	\\
	&	100	&	108.9	&	(3)	&		&	1000	&	4	&	(17)	&		&	2.17	&	5812.06	&	(2)	\\
	&	100	&	88.4	&	(6)	&		&	1100	&	1.85	&	(16)	&		&	2.2	&	4657.21	&	(1)	\\
	&	450	&	1.09	&	(12)	&		&	1100	&	3.5	&	(16)	&		&	2.2	&	4552.7	&	(3)	\\
	&	850	&	0.35	&	(12)	&		&	1136	&	3.5	&	(22)	&		&	3.5	&	2952.2	&	(3)	\\
	&	1200	&	0.13	&	(11)	&		&	1200	&	1.58	&	(11)	&		&	4.9	&	1323.7	&	(3)	\\
	&	1200	&	0.18	&	(19)	&		&	1200	&	3.8	&	(19)	&		&	12	&	908	&	(6)	\\
	&	1300	&	0.12	&	(13)	&		&	1300	&	1.52	&	(18)	&		&	12	&	729.6	&	(3)	\\
\cline{1-4}										\cline{5-8}																			
	&		&		&				&		&		&		&				&		&	25	&	437	&	(6)	\\
\par
%\end{tabular}
%\end{table}