\begin{table}%ta.5
%\centering
\par
\caption{\label{rmon}Table of fluxes for R~Mon.}  
\small \begin{tabular}{lllll}
\hline\hline \noalign{\smallskip}
Wavelength ($\mu$m) & Flux (Jy) & Flux error (Jy) & Beam size ($''$) & Reference/Flux type \\
\hline 
1.235 & 0.213 & 0.005 & 2 & BAND$\_$J$\_$2MASS \\
1.256 & 0.027 & 0.0010 & 6 & Close (1997) \\
1.633 & 0.25 & 0.01 & 6 & Close (1997) \\
1.662 & 0.630 & 0.015 & 2 & BAND$\_$H$\_$2MASS \\
2.159 & 1.860 & 0.040 & 2 & BAND$\_$Ks$\_$2MASS \\
2.210 & 0.99 & 0.01 & 6 & Close (1997) \\
3.163 & 11.17 & 0.01 & 6 & Close (1997) \\
3.600 & 18 & 0 & 12 & Audard (2007) \\
3.930 & 19.69 & 0.01 & 6 & Close (1997) \\
4.290 & 21.05 & 0.01 & 18.3 & BAND$\_$B1$\_$MSX6C \\
4.350 & 29.16 & 0.01 & 18.3 & BAND$\_$B2$\_$MSX6C \\
4.674 & 23.85 & 0.01 & 6 & Close (1997) \\
5.800 & 30.41 & 0.4 & 12 & Audard (2007) \\
8.000 & 31 & 0 & 12 & Audard (2007) \\
8.280 & 32.09 & 0.01 & 18.3 & BAND$\_$A$\_$MSX6C \\
11.700 & 46.59 & 0.01 & 6 & Close (1997) \\
12.000 & 58.3 & 0.1 & 30 & Hillenbrand (1992, IRAS) \\
12.130 & 47.18 & 0.01 & 18.3 & BAND$\_$C$\_$MSX6C \\
14.650 & 58.53 & 0.01 & 18.3 & BAND$\_$D$\_$MSX6C \\
20.800 & 103.1 & 0.1 & 6 & Close (1997) \\
21.340 & 102.2 & 0.01 & 18.3 & BAND$\_$E$\_$MSX6C \\
25.000 & 139.0 & 1.0 & 30 & Hillenbrand (1992, IRAS) \\
52.560 & 99 & 4 & 30 & Spitzer .tbl file \\
69.660 & 81 & 3 & 30 & Spitzer .tbl file \\
93.600 & 62.3 & 2.0 & 30 & Spitzer .tbl file \\
350 & 2 & 0.300 & 18.5 & Mannings (1994) \\
450 & 1.56 & 0.25 & 18.3 & Mannings (1994) \\
800 & 0.220 & 0.040 & 17.0 & Mannings (1994) \\
1100 & 0.077 & 0.018 & 18.8 & Mannings (1994) \\
1200 & 0.049 & $10^{-4}$ & 11 & Our data -- 30~m bolometer map \\
1300 & 0.079 & 0.019 & 19.8 & Mannings (1994) \\
1400 & 0.0118 & 0.0020 & $0.72\times0.33$ & Our data \\
2700 & 0.0041 & $5.0 \times 10^{-4}$ & $1.28\times0.83$ & Our data \\
7000 & $1.26\times 10^{-3}$ & $1.3\times10^{-4}$ & $2.21\times1.66$ & Our data \\
13~000 &$ 7.8\times 10^{-4}$ & $1.0\times10^{-4}$ & $5.18 \times 3.19$ & Our data \\
20~000 &$ 5.9\times 10^{-4}$ & $3.0\times10^{-4}$ & 1.4 & Skinner (1993) \\
36~000 &$ 4.0\times 10^{-4}$ & $1.0\times10^{-4}$ & 0.3 & Skinner (1993) \\
60~000 &$ 2.9\times 10^{-4}$ & $1.0\times10^{-4}$ & 4.3 & Skinner (1993) \\
\hline
\end{tabular}
\end{table}