\begin{table}%t2
%\centering
\par
\caption{Literature infrared photometry used in this work. 
Columns~3--7 list the magnitudes in the $J$~(1.25~$\mu$m),
$H$~(1.65~$\mu$m), $K$~(2.2~$\mu$m), $L$~(3.6~$\mu$m), and $M$~(4.8~$\mu$m)
photometric bands, with references in Col.~8. The listed reference 
codes are:
 BO:  \citet{1991AetAS...91..409B};
 CA:   \citet{1990MNRAS.242....1C};
 CO:   \citet{1973MNRAS.161...97C};
 CU:   \citet{2003yCat.2246....0C};
 DW:   \citet{2001AetA...380..609D};
DW2:   \citet{1996AetAS..119....1D};
 EI:  \citet{2001AetA...365..110E};
 FO:   \citet{1992AetAS...93..151F};
 GL: \citet{1974MNRAS.167..237G};
 HI:  \citet{1992ApJ...397..613H};
 LA:   \citet{1990AJ.....99.1232L};
 MA:  \citet{1998AetA...331..211M};
 ME:   \citet{1967BOTT....4..149M};
 ST:   \citet{1990ApJ...362..168S};
 SY:   \citet{1996MNRAS.279..915S};
 VR: \citet{1976AJ.....81..317V};
 WA:  \citet{1988AetA...203..348W}.
Columns~9--12 contain the infrared fluxes in Jy from the IRAS Point Source
Catalogue \citep{1988IRASP.C......0J}.
%For T CrA we use an observation of the Kuiper
%Airborne Observatory \citep{1985ApJ...293..165W}.
%IP: \cite{1988IRASP.C......0J},
%WI: \cite{1985ApJ...293..165W}).
}
\label{tab:t2_fs:literature_photometry}
\par
\begin{tabular}{rlccccclrrrr}
\hline\hline
(1) & \ \ \ \ (2) & \ \ \ \ (3) & \ (4) & \ (5) & (6) \ & \ \ \ \ (7) & \ (8) &
\ (9) & \ \ \ \ (10)& (11) & (12) \\ % & (12) \\
\# & star       &  $J$  & $H $ & $K$  & $L$ & $M$   & References  & 12~$\mu$m & 25~$\mu$m  & 60~$\mu$m & 100~$\mu$m \\ %& ref \\
\hline
% omit=['HD~143006','CD-42 11721','HR 4796','HD~141569','HD~140863','HD~50138',$
%       'HD~41511','HD~45677','V* R CRA','* BET PIC']
\par
  1& AB Aur        & 6.10  &  5.10 &  4.40 &  3.30 &  2.90 & HI                    &   27.16  &      48.10  &     105.60  &     114.10  \\ % & IP  \\
  2& UX Ori        & 8.03  &  7.43 &  6.71 &  5.61 &  5.32 & DW, 26.2.1986          &    2.68  &       3.69  &       2.85  & $\sim$3.76  \\ % & IP  \\
%  & HD~34282      & 9.17  &  8.32 &  7.42 &  6.25 &  6.16 & MA                    &    0.70  &       1.63  &      10.40  &      10.72  \\ % & IP  \\
  3& HD~36112      & 7.44  &  6.70 &  5.90 &  4.75 &  4.47 & MA                    &    5.59  &      12.59  &      27.98  &      18.95  \\ % & IP  \\
  4& HK Ori        & 9.52  &  8.38 &  7.29 &  5.87 &  5.10 & HI                    &    3.80  &       4.08  &    $<$1.64  &   $<$70.37  \\ % & IP  \\
%  & HD~36917      & 7.13  &  7.00 &  6.40 &  5.30 &  3.80 & MA                    &    5.73  & $\sim$3.37  &   $<$37.85  &  $<$740.10  \\ % & IP  \\
  5& HD~245185     & 9.34  &  8.87 &  8.26 &  7.46 &  6.23 & HI                    &    4.00  &       5.96  &       4.97  &       3.61  \\ % & IP  \\
%  & HD~36910      & 7.92  &  7.47 &  6.45 &  4.90 &  4.20 & J CU; H GL; K-M CO    &    6.21  &      20.66  &      21.88  &      13.65  \\ % & IP  \\
  6&  V380 Ori     & 8.25  &  7.10 &  6.03 &  4.44 &  3.61 & J-L ST;  M ME         &    8.61  &       8.85  &   $<$75.90  &   $<$38.59  \\ % & IP  \\
  7& HD~37357      & 8.31  &  7.88 &  7.24 &  6.33 &       & MA                    &    2.01  &       2.79  & $\sim$2.90  &$\sim$20.29  \\ % & IP  \\
  8& HD~37806      & 7.38  &  6.68 &  5.77 &  4.23 &  3.79 & MA                    &   11.02  &       9.40  &    $<$5.18  &   $<$33.98  \\ % & IP  \\
%  & Beta Pic      & 3.58  &  3.49 &  3.48 &  3.48 &  3.46 & J-L CA; M BO          &    3.46  &       9.05  &      19.90  &      11.28  \\ % & IP  \\
%  & HD~41511      & 2.93  &  2.09 &  1.67 &  0.85 &  0.59 & MA                    &  143.50  &      72.24  &      14.52  &       3.77  \\ % & IP  \\
%  & HD~45677      & 7.76  &  6.65 &  4.79 &  1.97 &  1.15 & J-K DW2;  L,M FO      &  146.30  &     143.40  &      24.80  &       5.87  \\ % & IP  \\
%  & HD~50138      & 5.83  &  5.14 &  4.20 &  2.81 &  2.20 & DW                    &   70.28  &      62.55  &      13.27  &       2.81  \\ % & IP  \\
%  & HD~85567      & 7.58  &  6.78 &  5.84 &  4.41 &  3.93 & MA                    &    6.39  &       5.81  &       1.40  & $\sim$8.84  \\ % & IP  \\
  9& HD~95881      & 7.50  &  6.79 &  5.87 &  4.28 &  3.71 & MA                    &    9.14  &       6.87  &       1.45  &    $<$1.09  \\ % & IP  \\
 10& HD~97048      & 7.30  &  6.75 &  6.04 &  4.61 &  4.56 & HI                    &   14.49  &      40.34  &      69.91  &  $<$250.10  \\ % & IP  \\
%  & HD~98922      & 6.15  &  5.36 &  4.41 &  2.80 &  2.24 & MA                    &   40.16  &      27.24  &       6.19  &    $<$7.96  \\ % & IP  \\
 11& HD~100453     & 6.97  &  6.32 &  5.52 &  4.20 &  3.79 & MA                    &    7.23  &      33.59  &      39.36  &      23.86  \\ % & IP  \\
 12& HD~100546     & 6.43  &  5.88 &  5.20 &  4.15 &  3.80 & MA                    &   65.78  &     242.60  &     165.20  &      98.56  \\ % & IP  \\
 13& HD~101412     & 8.70  &  8.24 &  7.25 &  5.81 &  5.08 & DW                    &    3.22  &       3.09  & $\sim$1.69  &$\sim$10.52  \\ % & IP  \\
 14& HD~104237     & 5.75  &  5.14 &  4.42 &  3.05 &  2.58 & MA                    &   23.65  &      23.05  &      14.72  &       9.58  \\ % & IP  \\
%  & HR 4796       &       &       &       &       &       &                       & $<$0.43  & $\sim$3.38: & $\sim$7.36  &       3.81  \\ % & IP  \\
 15& HD~135344     & 7.44  &  6.72 &  5.96 &  4.76 &  4.69 & MA                    &    1.59  &       6.71  &      25.61  &      25.69  \\ % & IP  \\
 16& HD~139614     & 7.75  &  7.34 &  6.76 &  5.68 &  5.49 & MA                    &    4.11  &      18.14  &      19.30  &      13.94  \\ % & IP  \\
%  & HD~140863     & 9.50  &  9.45 &  9.48 &       &       & MA                    &    5.29  &       6.58  &       1.14  &   $<$40.17  \\ % & IP  \\
%  & HD~141569     & 6.87  &  6.84 &  6.80 &  6.67 &  6.50 & SY                    &    0.55  &       1.87  &       5.53  &       3.47  \\ % & IP  \\
 17& HD~142666     & 7.34  &  6.72 &  6.04 &  4.97 &  4.69 & MA                    &    8.57  &      11.21  &       7.23  &       5.46  \\ % & IP  \\
 18& HD~142527     & 6.65  &  5.94 &  5.20 &  3.89 &  3.50 & MA                    &   10.38  &      21.23  &     105.10  &      84.70  \\ % & IP  \\
%  & HD~143006     & 8.35  &  7.65 &  7.06 &  6.14 &  6.18 & SY                    &    0.86  &       3.16  &       6.57  &       4.82  \\ % & IP  \\
 19& HD~144432     & 7.21  &  6.69 &  6.14 &  5.14 &  4.90 & MA                    &    7.53  &       9.36  &       5.76  &       3.29  \\ % & IP  \\
 20& HD~144668     & 5.83  &  5.18 &  4.38 &  3.08 &  2.54 & HI                    &   18.05  &      14.51  &$\sim$14.36  &   $<$63.25  \\ % & IP  \\
 21& HD~150193     & 7.05  &  6.37 &  5.64 &  4.37 &  3.93 & MA                    &   17.61  &      18.10  &       8.13  &   $<$16.25  \\ % & IP  \\
%  & CD-42 11721   & 7.33  &  5.97 &  4.51 &  2.39 &  1.70 & HI                    &   94.91  &     251.90  &    1918.00  &    2213.00  \\ % & IP  \\
%  & 51 Oph        & 4.61  &  4.53 &  4.31 &  3.46 &  2.60 & WA                    &   15.67  &      10.19  &       1.06  &    $<$5.97  \\ % & IP  \\
 22& HD~163296     & 6.24  &  5.52 &  4.70 &  3.52 &  3.14 & MA                    &   18.20  &      20.99  &      28.24  &   $<$40.62  \\ % & IP  \\
 23& HD~169142     & 7.43  &  7.01 &  6.53 &  5.64 &  5.57 & MA                    &    2.95  &      18.43  &      29.57  &      23.42  \\ % & IP  \\
%  & R CrA         & 7.92  &  5.61 &  3.80 &  2.03 &  0.98 & HI                    &  111.10  &     221.50  &     608.20  &    1206.00  \\ % & IP  \\
%  & T CrA         & 8.90  &  7.52 &  6.34 &  5.01 &  4.17 & J-L GL; M VR          &    9.36  &      38.33  &      76.10  &      40.00  \\ % & WI  \\
 24& HD~179218     & 6.99  &  6.64 &  5.91 &  4.68 &  4.18 & J, H EI; K-M LA        &   23.44  &      43.63  &      29.92  &      17.35  \\ 
\hline
\end{tabular}
\end{table}