\begin{table}%t5
%\centering
\par
\caption {\label{tab:extinction}Different estimates of the $J$-band extinction for the objects 
in our sample, and adopted values (cf. Sect.~\ref{sect:extinction}).}
$$
\begin{tabular}{lrr@{}lr@{}lr}
\hline\hline
\scriptsize
&\multicolumn{6}{c}{$A_J$ [mag]}\\
\cline{2-7}
        Name &                          Lit. &     \multicolumn{2}{c}{$N_{\rm H}$} &       \multicolumn{2}{c}{SED} &   Adopted \\
\hline
 DoAr25/GY17 &       0.7 &            1.7 & $_{       1.6}^{       1.8}$ &            0.5 & $_{       0.2}^{       0.8}$ &       0.7 \\
 IRS14/GY54  &       5.2 &                                             & &            5.0 & $_{       4.9}^{       5.0}$ &       5.2 \\
 WL12/GY111  &           &           26.1 & $_{      12.7}^{      70.0}$ &           15.8 & $_{      12.8}^{      17.7}$ &      15.8 \\
 WL22/GY174  &           &           25.2 & $_{      19.2}^{      32.7}$ &           17.9 & $_{      17.4}^{     456.7}$ &      25.2 \\
 WL16/GY182  &      10.0 &                                             & &            8.6 & $_{       7.8}^{       9.2}$ &      10.0 \\
 WL17/GY205  &      11.3 &            6.7 & $_{       3.9}^{      10.5}$ &           11.9 & $_{      11.1}^{      13.0}$ &      11.3 \\
 WL10/GY211  &       4.5 &            5.0 & $_{       4.1}^{       5.9}$ &            4.5 & $_{       4.2}^{       4.7}$ &       4.5 \\
 EL29/GY214  &           &           11.4 & $_{      10.4}^{      12.8}$ &           11.9 & $_{      10.5}^{      12.6}$ &      11.4 \\
 GY224       &       8.6 &            6.1 & $_{       4.7}^{       8.0}$ &           10.2 & $_{       9.8}^{      10.6}$ &       8.6 \\
 WL19/GY227  &      16.3 &           17.7 & $_{      15.1}^{      20.6}$ &           14.9 & $_{      14.8}^{      15.4}$ &      16.3 \\
 WL11/GY229  &       4.3 &                                             & &            5.2 & $_{       5.0}^{       5.3}$ &       4.3 \\
 WL20/GY240  &           &            4.1 & $_{       3.9}^{       4.3}$ &            6.7 & $_{       6.0}^{       9.9}$ &       4.1 \\
 IRS37/GY244 &           &           10.4 & $_{       7.1}^{      15.7}$ &           11.8 & $_{      10.8}^{      12.7}$ &      10.4 \\
 WL5/GY246   &      16.8 &           11.8 & $_{      10.6}^{      13.0}$ &           14.5 & $_{      12.3}^{      18.3}$ &      16.8 \\
 IRS42/GY252 &       7.5 &            7.0 & $_{       4.8}^{       9.3}$ &            8.3 & $_{       8.2}^{      11.9}$ &       7.5 \\
 GY253       &       8.8 &            6.1 & $_{       5.7}^{       6.5}$ &            8.1 & $_{       7.9}^{       8.3}$ &       8.8 \\
 WL6/GY254   &      18.6 &           10.2 & $_{       7.5}^{      13.1}$ &           14.9 & $_{      14.2}^{      18.4}$ &      18.6 \\
 CRBR85      &           &                                             & &           19.0 & $_{      18.6}^{      19.6}$ &      19.0 \\
 IRS43/GY265 &           &            8.2 & $_{       7.9}^{       8.5}$ &           13.4 & $_{      12.5}^{      14.4}$ &       8.2 \\
 IRS44/GY269 &           &           12.8 & $_{      12.2}^{      13.5}$ &           16.1 & $_{      14.5}^{      17.8}$ &      12.8 \\
 IRS45/GY273 &       6.6 &            1.8 & $_{       0.6}^{       3.3}$ &            8.3 & $_{       7.7}^{       8.9}$ &       6.6 \\
 IRS46/GY274 &           &           15.1 & $_{      10.1}^{      23.6}$ &            9.1 & $_{       8.4}^{       9.6}$ &      15.1 \\
 IRS47/GY279 &       7.4 &            3.5 & $_{       2.3}^{       5.2}$ &            8.7 & $_{       8.3}^{       9.4}$ &       7.4 \\
 GY289       &       7.3 &            3.5 & $_{       3.0}^{       3.9}$ &            6.6 & $_{       6.1}^{       7.0}$ &       7.3 \\
 GY291       &       7.4 &            4.2 & $_{       3.6}^{       4.7}$ &            6.9 & $_{       6.6}^{       7.2}$ &       7.4 \\
 IRS48/GY304 &           &                                             & &            7.4 & $_{       5.0}^{       9.9}$ &       7.4 \\
 IRS51/GY315 &      12.9 &            6.2 & $_{       5.5}^{       6.8}$ &            8.6 & $_{       7.6}^{       9.2}$ &      12.9 \\
 IRS54/GY378 &       6.2 &           35.8 & $_{      11.6}^{      76.5}$ &            7.4 & $_{       7.0}^{       7.9}$ &       6.2 \\
\hline
\end{tabular}
$$
\end{table}