\begin{table}%t3
 \caption{\label{table:3}Mid-IR, far-IR, and submm photometry of all BPMG members that have been observed at submm wavelengths. A~$3\sigma$ upper limit on the flux density is given for non-detections.}
%\centering
\small
\begin{tabular}{l c c c c c}
\hline\hline \noalign{\smallskip}
Star & Other name & Instrument & $\lambda$ & $F_{\nu}$ & Reference\\
 &  &  & ($\mu$m) & (Jy) &  \\
 \hline
HD~15115 &  & MIPS & 24 & $0.054\pm0.006$ & 1\\
 &  & IRAS & 60 & $0.473\pm0.052$ & 1\\
 &  & ISOPHOT & 60 & $0.415\pm0.020$ & 1\\
 &  & ISOPHOT & 90 & $0.427\pm0.030$ & 1\\
 &  & SCUBA & 850 & $0.0049\pm0.0016$ & 2\\
 &  & LABOCA & 870 & ${<}0.0153$ & 3\\
HD~35850 & AF~Lep & MIPS & 24 & $0.0790\pm0.00316$ & 4\\ 
 &  & MIPS & 70 & $0.0447\pm0.00447$ & 4\\
 &  & MIPS & 160 & ${<}0.077$ & 4\\
 &  & IRAS & 12 & $0.4900\pm0.0588$ & 5, 6\\
 &  & IRAS & 25 & $0.080\pm0.008$ & 5, 6\\
 &  & IRAS & 60 & ${<}0.180$ & 5, 6\\
 &  & IRAS & 100 & ${<}1.930$ & 5, 6\\
 &  & ISOPHOT & 60 & $0.049\pm0.014$ & 5, 6\\
 &  & ISOPHOT & 90 & $0.050\pm0.012$ & 5, 6\\
 &  & SCUBA & 850 & ${<}0.0045$ & 7\\
HD~39060 & $\beta$~Pic & MIPS & 24 & $7.276\pm0.29104$ & 4\\
 &  & MIPS & 70 & $12.990\pm1.299$ & 4\\
 &  & MIPS & 160 & $3.646\pm0.43752$ & 4\\
 &  & IRAS & 12 & $2.38\pm0.10$ & 1\\
 &  & IRAS & 25 & $10.29\pm0.41$ & 1\\
 &  & IRAS & 60 & $18.92\pm0.76$ & 1\\
 &  & IRAS & 100 & $9.32\pm0.37$ & 1\\
 &  & ISOPHOT & 60 & $14.7\pm0.346$ & 8\\
 &  & ISOPHOT & 120 & $6.680\pm1.010$ & 1\\
 &  & ISOPHOT & 150 & $4.390\pm0.670$ & 1\\
 &  & ISOPHOT & 170 & $3.807\pm0.143$ & 1\\
 &  & ISOPHOT & 200 & $2.030\pm0.340$ & 1\\
 &  & SCUBA & 850 & $0.0583\pm0.0065$ & 9\\
 &  & LABOCA & 870 & $0.0636\pm0.0067$ & 3\\
 &  & SIMBA & 1200 & $0.0243\pm0.003$ & 10\\
 &  & SEST & 1300 & $0.0249\pm0.0026$ & 16\\
HD~164249 &  & MIPS & 24 & $0.076\pm0.0304$ & 4\\ 
 &  & MIPS & 70 & $0.624\pm0.0624$ & 4\\
 &  & MIPS & 160 & $0.104\pm0.01248$ & 4\\
 &  & IRAS & 12 & $0.280\pm0.028$ & 11\\
 &  & IRAS & 25 & ${<}0.158\pm$ & 11\\
 &  & IRAS & 60 & $0.669\pm0.094$ & 1\\
 &  & IRAS & 100 & ${<}2.63$ & 11\\
 &  & ISOPHOT & 60 & $0.761\pm0.0380$ & 1\\
 &  & ISOPHOT & 90 & $0.560\pm0.0390$ & 1\\
 &  & LABOCA & 870 & ${<}0.012$ & 3\\
HD~172555 &  & MIPS & 24 & $0.766\pm0.03064$ & 4\\ %fix ref from here
 &  & MIPS & 70 & $0.197\pm0.0197$ & 4\\
 &  & IRAS & 12 & $1.34\pm0.05$ & 1\\
 &  & IRAS & 25 & $0.91\pm0.05$ & 1\\
 &  & IRAS & 60 & $0.241\pm0.036$ & 1\\
 &  & LABOCA & 870 & $0.07\pm0.01$ & 3\\
HD~181296 & $\eta$~Tel & MIPS & 24 & $0.382\pm0.01528$ & 4\\
 &  & MIPS & 70 & $0.409\pm0.0409$ & 4\\
 &  & MIPS & 160 & $0.068\pm0.00816$ & 4\\
 &  & IRAS & 12 & $0.351\pm0.018$ & 1\\
 &  & IRAS & 25 & $0.496\pm0.025$ & 1\\
 &  & IRAS & 60 & $0.449\pm0.040$ & 1\\
 &  & ISOPHOT & 60 & $0.433\pm0.022$ & 1\\
 &  & ISOPHOT & 90 & $0.286\pm0.021$ & 1\\
 &  & LABOCA & 870 & ${<}0.0144$ & 3\\
\hline
HD~181327 &  & MIPS & 24 & $0.195\pm0.0078$ & 4\\
 &  & MIPS & 70 & $1.468\pm0.1468$ & 4\\
 &  & MIPS & 160 & $0.658\pm0.07896$ & 4\\
 &  & IRAS & 12 & $0.164\pm0.016$ & 11\\
&  & IRAS & 25 & $0.286\pm0.023$ & 1\\
 &  & IRAS & 60 & $1.93\pm0.08$ & 1\\
 &  & IRAS & 100 & $1.69\pm0.20$ & 1\\
 &  & ISOPHOT & 60 & $1.730\pm0.170$ & 1\\
 &  & ISOPHOT & 90 & $1.410\pm0.140$ & 1\\
&  & ISOPHOT & 170 & $0.736\pm0.192$ & 1\\
 &  & LABOCA & 870 & $0.0517\pm0.0062$ & 3\\
HD~191089 &  & MIPS & 24 & $0.1856\pm0.0076$ & 12\\
 &  & MIPS & 70 & $0.5443\pm0.0401$ & 12\\
 &  & MIPS & 160 & $0.2046\pm0.0446$ & 12\\
 &  & IRAS & 25 & $0.387\pm0.058$ & 1\\
 &  & IRAS & 60 & $0.729\pm0.058$ & 1\\
 &  & ISOPHOT & 60 & $0.781\pm0.081$ & 1\\
 &  & ISOPHOT & 90 & $0.370\pm0.038$ & 1\\
 &  & LABOCA & 870 & ${<}0.018$ & 3\\
HD~196982 & AT~Mic & MIPS & 24 & $0.1160\pm0.00464$ & 4\\
 &  & MIPS & 70 & ${<}0.018$ & 4\\
 &  & SCUBA & 850 & ${<}0.009$ & 7\\
HD~197481 & AU~Mic & MIPS & 24 & $0.1430\pm0.00572$ & 4\\
 &  & MIPS & 70 & $0.2050\pm0.0205$ & 4\\
 &  & MIPS & 160 & $0.1680\pm0.0202$ & 4\\
 &  & IRAS & 60 & $0.252\pm0.043$ & 1\\
 &  & SHARC & 350 & $0.072\pm0.020$ & 13, 15\\
 &  & SCUBA & 450 & $0.085\pm0.042$ & 7\\
 &  & SCUBA & 850 & $0.0144\pm0.0018$ & 7\\
HD~199143 &  & MIPS & 24 & $0.0350\pm0.00014$ & 4\\
 &  & MIPS & 70 & ${<}0.022$ & 4\\
 &  & MIPS & 160 & ${<}0.031$ & 4\\
 &  & SCUBA & 850 & ${<}0.0075$ & 7\\
HD~358623 & AZ~Cap & MIPS & 24 & $0.0130\pm0.00052$ & 4\\
 &  & MIPS & 70 & ${<}0.0012$ & 4\\
 &  & SCUBA & 850 & ${<}0.0069$ & 7\\
\hline
\end{tabular}
\medskip
References. (1)~\citet{Moor2006}; (2) \citet{Williams2006}; (3) this paper; (4)~\citet{Rebull2008}; (5)~\citet{Spangler2001}; (6)~\citet{Silverstone2000}; (7)~\citet{Liu2004}; (8)~\citet{Habing2001}; (9)~\citet{Holland1998}; (10)~\citet{Liseau2003}; (11)~\citet{Moshir1993}; (12)~\citet{Hillenbrand2008a}; (13)~\citet{Chen2005}; (14)~\citet{diFrancesco2008}; (15)~\citet{Augereau2006}; (16)~\citet{Chini1991}.
\end{table}