\begin{table}%t1
%\centering
\par
\caption{Hot post-AGB stars.}\label{t1}
\begin{tabular}{cccccccccc}
\hline \hline
Star No. & IRAS & Name & Optical & $l$ & $b$ & \multicolumn{4}{c}{IRAS fluxes (Jy.)} \\ \cline{7-10} 
         &      &      & Sp. type &  &   & 12~$\mu$ & 25~$\mu$ & 60~$\mu$ & 100~$\mu$ \\
\hline 
1. & 12584--4837 & Hen3--847     & Be$^{1}$ & 304.60&  +13.95& 36.07 & 48.75 & 13.04 & 3.31 \\
2. & 13266--5551 & -55 5588     & B1Ibe   & 308.30&  +6.36 & 0.76  & 35.90 & 35.43 & 11.66\\
3. & 14331--6435 & Hen3--1013    & B3Ie    & 313.89&  $-$4.20 & 4.04  & 108.70& 70.71 & 20.61\\
4. & 16206--5956 & SAO 243756   & A0Ia$^{2}$ & 326.77&  $-$7.49 & 0.36L & 11.04 & 12.30 & 4.83\\ 
5. & 17203--1534 &              & B1IIIpe & 8.55  &  +11.49& 0.32  & 10.70 & 6.88  & 3.37\\    
6. & 17311--4924 & Hen3--1428    & B1IIe   & 341.41&  $-$9.04 & 18.34 & 150.70& 58.74 & 17.78\\ 
7. & 17423--1755 & Hen3--1475    & Be      &  9.36&  +5.78 &  7.05 &  28.31& 63.68 & 33.43\\ 
8. & 17460--3114 &  SAO 209306  & O8III   & 358.42&  $-$1.88 & 6.26  & 20.82 & 12.20 &220.40L\\
9. & 18023--3409 & LSS 4634     & B2IIIe  & 357.61&  $-$6.31 & 0.26L & 2.94  & 1.82  & 25.64L\\ 
10.& 18062+2410 & SAO 85766    & B1I$^{3}$ & 50.67&  +19.79& 3.98  & 19.62 & 2.90 & 1.00L \\  
11.& 18371--3159 & LSE 63       & B1Iabe  & 2.92 & $-$11.82 & 0.25L &  6.31 &  5.16 & 1.95\\
12.& 18379--1707 & LSS 5112     & B1IIIpe & 16.50 & $-$5.42  & 1.67  & 23.76 &  7.12 & 3.66L\\
13.& 19590--1249 & LSIV--12 111  & B1Ibe   & 29.18 & $-$21.26 & 0.29: & 10.26 & 6.45 & 1.77: \\
14.& 22023+5249 & LSIII +5224  & B$^{4}$ & 99.30 &  $-$1.96 & 1.02  & 24.69 & 14.52 & 3.93L\\
15.& 22495+5134 & LSIII +5142  & PN$^{5}$ & 104.84&  $-$6.77 & 0.54  & 12.37 &  7.18 & 3.12\\ 
\hline
\end{tabular}
A colon {:} indicates moderate quality IRAS flux,
{L} is for an upper limit.\\
The spectral types are from Parthasarathy et~al.
(2000a) except $^{1}$ Kazarovets et~al. (\cite{Kaz00}); $^{2}$ Schild et~al. (\cite{Schi83});
$^{3}$ Parthasarathy et~al. (\cite{Par00b}b); $^{4}$ Simbad database; $^{5}$ Acker et~al. (\cite{Ack92}).
\end{table}