\begin{table}%[!htp]%t4
\caption{\label{bbfit}Comparison between $A_{J}$, and our SED blackbody temperature fitting with those from \citet{LR99} for the $\rho$~Oph~sources.}
%\centerline
{
\begin{tabular}{ccccc}
\hline
\hline
\multicolumn{1}{c}{} & \multicolumn{2}{c}{SED fitting$^{a}$} & 
\multicolumn{2}{c}{$K-$band}\\
&&&\multicolumn{2}{c}{spectroscopy$^{b}$} \\
\hline
Sources & $A_{J}$ & $T_{\rm bb}$ & $A_{J}$ & 
$T_{\rm eff}$ \\
\hline
GY12    & 5.02--5.23 & 3549--3925   & 4.6   & 3955  \\
GY135   & 3.61--3.64 & 4323--4690   & 4.4   & 4205  \\
GY156   & 5.05--5.22 & 4268--4733   & 6.1   & 3955  \\
LFAM8   & 5.51--5.81 & 3434--3873   & 6.6   & 3595  \\
VSSG11  & 3.50--3.51 & 3894--4262   & 4.0   & 3850  \\
B162607 & 4.98--5.11 & 3533--4103   & \ldots &\ldots \\
S1      & 3.57--3.81 & 17665--19935 & \ldots & 18~700 \\
DoAr21  & 1.80--1.97 & 4614--4929   & 1.6    & 5080  \\
SR20    & 2.47--2.53 & 3677--3945   & 2.1    & 3955   \\
GY289   & 6.39--6.81 & 3910--4420   &\ldots  &\ldots \\
IRS~55   & 1.41--1.51   & 3950--4175   &\ldots  &\ldots \\
WL5     & 12.26--13.93 & 5775--6970   &\ldots  &\ldots \\
SR12    & 0.21--0.22   & 3610--3640   & 0.20   & 3850  \\
GY112   & 0.96--1.05   & 3505--3745   &\ldots  &\ldots \\
GY193   & 1.80--1.87   & 3360--3650   &\ldots  &\ldots \\
GY194   & 2.19--2.24   & 3550--3865   &\ldots  &\ldots \\
GY253   & 7.08--7.59   & 3350--3820   & 8.2    & 3350  \\
GY410   & 2.51--2.53   & 3870--4120   & 2.7    & 4060  \\
B162730 & 2.44--2.49   & 3555--3850   &\ldots  &\ldots \\
WL19    & 14.46--16.45 & 6000--7210   &\ldots  &\ldots \\
\hline
\end{tabular}}
\smallskip
$^{a}$ This work; $^{b}$ \citet{LR99}.
\end{table}