\begin{table}%C.4
%\centering
\par
\caption{IRAS photometry points at $12$, $25$, $60$ and
$100~\mu$m. Note however that in some cases the data points are upper
limits (L); these observations are probably contaminated by
interstellar cirrus clouds. Other data are lower limits (:). Remark
also that for BD$+$39$^{\circ}$4926 we don't have IRAS
datapoints.\label{DATA:IRAS}}
\begin{tabular}{llllll}
\hline
\hline
No	&Name			&$F_{12}$ (Jy)	&$F_{25}$ (Jy)	&$F_{60}$ (Jy)	&$F_{100}$ (Jy)\\
	&			&$12~\mu$m	&$25~\mu$m	&$60~\mu$m	&$100~\mu$m\\
\hline
1	&TW~Cam		&8.25		&5.60		&1.84		&1.79L\\
\par
2	&RV~Tau		&22.52		&18.05		&6.50		&2.44:\\
\par
3	&IRAS~05208		&9.53		&9.30		&2.78		&1.40\\
\par
4	&DY~Ori		&12.43		&14.89		&4.18		&11.46L\\
\par
5	&CT~Ori		&6.14		&5.55		&1.24		&1.59L\\
\par
6	&SU~Gem		&7.91		&5.68		&2.19		&11.99L\\
\par
7	&UY~CMa		&3.49		&2.46		&0.57		&1.00L\\
\par
8	&HD~44179		&421.60		&456.10		&173.10		&66.19\\
\par
9	&HD~46703		&0.46		&0.38:		&0.40L		&1.15L\\
\par
10	&ST~Pup		&3.51		&5.92		&1.24		&1.13L\\
\par
11	&HD~52961		&4.53		&2.22		&0.95		&0.87:\\
\par
12	&SAO~173329		&2.28		&1.83		&0.64		&10.45L\\
\par
13	&U~Mon			&124.30		&88.43		&26.59		&9.54\\
\par
14	&AR~Pup		&131.30		&94.32		&26.12		&11.96:\\
\par
15	&IRAS~08544		&180.30		&158.80		&56.25:		&28.43L\\
\par
16	&IRAS~09060		&3.78		&2.53		&0.65		&1.00L\\
\par
17	&IRAS~09144		&15.31		&12.14		&2.86		&24.68L\\
\par
18	&IW~Car		&101.00		&96.24		&34.52		&13.46\\
\par
19	&IRAS~09400		&7.85		&5.48		&1.58		&8.34L\\
\par
20	&IRAS~09538		&2.33		&1.60		&0.53		&1.34L\\
\par
21	&HR~4049		&48.25		&9.55		&1.77		&1.69L\\
\par
22	&IRAS~10174		&41.80		&60.39		&16.13:		&174.30L\\
\par
23	&IRAS~10456		&189.10		&115.50		&30.86		&10.89\\
\par
24	&HD~95767		&22.13		&15.65		&10.90		&58.88\\
\par
25	&GK~Car		&2.85		&2.45		&0.79		&12.41L\\
\par
26	&IRAS~11472		&11.35		&14.18		&1.78		&1.00L\\
\par
27	&RU~Cen		&5.32		&10.96		&5.65		&2.09\\
\par
28	&SX~Cen		&5.92		&3.59		&1.10		&1.55L\\
\par
29	&HD~108015		&32.46		&33.23		&7.99		&2.41\\
\par
30	&IRAS~13258		&1.90		&2.97		&1.46		&3.82:\\
\par
31	&EN~TrA		&13.20		&10.30		&4.11		&2.12\\
\par
32	&IRAS~15469		&48.81		&42.12		&15.50		&278.10L\\
\par
33	&IRAS~15556		&19.86		&17.80		&7.10		&189.80L\\
\par
34	&IRAS~16230		&4.29		&3.34		&0.82		&14.55L\\
\par
35	&IRAS~17038		&8.05		&9.67		&4.49		&43.34L\\
\par
36	&IRAS~17233		&17.02		&13.40		&3.67		&32.08L\\
\par
37	&IRAS~17243		&10.76		&8.77		&3.69		&5.41:\\
\par
38	&89~Her		&97.52		&54.49		&13.42		&6.04\\
\par
39	&AI~Sco		&17.59		&11.38		&2.95		&46.76L\\
\par
40	&IRAS~18123		&10.72		&11.02		&4.21		&1.85L\\
\par
41	&IRAS~18158		&3.00		&2.64		&1.03		&1.56L\\
\par
42	&AC~Her		&41.43		&65.33		&21.37		&8.04\\
\par
43	&AD~Aql		&2.49		&2.72		&0.65L		&24.46L\\
\par
44	&IRAS~19125		&28.89		&26.51		&7.81		&28.05L\\
\par
45	&EP~Lyr		&0.31L		&0.50		&0.40L		&2.10L\\
\par
46	&IRAS~19157		&8.88		&7.16		&2.45		&11.05L\\
\par
47	&IRAS~20056		&17.52		&18.01		&5.38		&2.84L\\
\par
48	&R~Sge			&10.60		&7.54		&2.12		&1.72L\\
\par
49	&V~Vul			&12.35		&5.69		&1.29		&7.25L\\
\par
50	&HD~213985		&5.57		&4.66		&2.11		&1.01L\\\hline
\end{tabular}
\end{table}