\begin{table}%t1
 \caption{Distance modulii and distances derived with the red-clump stars for
 the 49~fields used along this work, with each field covering 0.07~deg$^2$
 on the sky centred on the Galactic coordinates given in Cols.~(1) and~(2). The last eight fields are those in which $H$-band data were used to derive distances.}
\label{tabla1}
%\centering
\small
    \begin{tabular}{ccccc}
\hline \hline
$l$ ($^\circ$) & $b$ ($^\circ$) & $\mu$ (mag) & $D$ (kpc) & $\sigma$ (kpc)\\ 
\hline
   18 &  0.0& 14.01 $\pm$ 0.07&    6.317 $\pm$ 0.229&      0.47 \\    
   20 &  0.0& 13.68 $\pm$ 0.07&	 5.449 $\pm$ 0.199&      0.44 \\    
   21 &  0.0& 14.05 $\pm$ 0.09&	 6.455 $\pm$ 0.298&      0.51 \\    
   22 &  0.0& 13.95 $\pm$ 0.08&	 6.187 $\pm$ 0.238&      0.47 \\    
   26 &  0.0& 13.81 $\pm$ 0.07&	 5.778 $\pm$ 0.186&      0.41 \\    
   27 &  0.0& 13.71 $\pm$ 0.08&	 5.525 $\pm$ 0.216&      0.42 \\    
   28 &  0.0& 13.66 $\pm$ 0.11&	 5.392 $\pm$ 0.303&      0.52 \\  
   29 &  0.0& 13.62 $\pm$ 0.10&	 5.308 $\pm$ 0.258&      0.50 \\  
   20 & $-$0.5& 13.36 $\pm$ 0.08&	 4.704 $\pm$ 0.184&	0.65\\  
   20 &  0.5& 13.79 $\pm$ 0.08&	 5.719 $\pm$ 0.221&	0.51\\  
   26 & $-$0.5& 13.58 $\pm$ 0.08&	 5.211 $\pm$ 0.204&	0.52\\  
   26 &  0.5& 13.65 $\pm$ 0.12&	 5.366 $\pm$ 0.304&	0.54\\  
   27 & $-$0.5& 13.55 $\pm$ 0.08&	 5.126 $\pm$ 0.202&	0.56\\  
   27 &  0.5& 13.72 $\pm$ 0.10&	 5.536 $\pm$ 0.248&	0.49\\  
   5 &  1.0& 14.25 $\pm$ 0.07& 	 7.094 $\pm$ 0.217&	0.70\\
   6 &  1.0& 14.55 $\pm$ 0.08& 	 8.116 $\pm$ 0.267&	0.42\\
   7 &  1.0& 14.15 $\pm$ 0.08& 	 6.767 $\pm$ 0.235&	0.67\\
   7 & $-$1.0& 14.06 $\pm$ 0.07& 	 6.488 $\pm$ 0.206&	0.45\\
   8 &  1.0& 14.38 $\pm$ 0.09& 	 7.530 $\pm$ 0.313&	0.71\\
   9 &  1.0& 13.97 $\pm$ 0.09& 	 6.236 $\pm$ 0.254&	0.62\\
   10 &  1.0& 14.29 $\pm$ 0.10&	 7.197 $\pm$ 0.332&	0.62\\
   15 &  1.0& 13.55 $\pm$ 0.11&	 5.135 $\pm$ 0.257&	0.45\\
   15 & $-$1.0& 13.33 $\pm$ 0.09&	 4.626 $\pm$ 0.188&	0.54\\
   20 &  1.0& 13.95 $\pm$ 0.12&	 6.174 $\pm$ 0.365&	0.47\\
   20 & $-$1.0& 13.72 $\pm$ 0.13&	 5.555 $\pm$ 0.335&	0.54\\
   23 &  1.0& 13.49 $\pm$ 0.13&	 4.991 $\pm$ 0.305&	0.58\\
   25 &  1.0& 13.86 $\pm$ 0.11&	 5.906 $\pm$ 0.322&	0.48\\
   25 & $-$1.0& 13.86 $\pm$ 0.10&	 5.929 $\pm$ 0.276&	0.49\\
   26 & $-$1.0& 13.51 $\pm$ 0.12&	 5.028 $\pm$ 0.327&	0.56\\
   3 & $-$2.0& 14.21 $\pm$ 0.07& 	 6.943 $\pm$ 0.229&	0.48\\
   5 & $-$2.0& 14.10 $\pm$ 0.10& 	 6.603 $\pm$ 0.298&	0.48\\
   7 &  2.0& 14.08 $\pm$ 0.09& 	 6.542 $\pm$ 0.264&	0.54\\
   7 & $-$2.0& 14.31 $\pm$ 0.10& 	 7.277 $\pm$ 0.333&	0.49\\
   10 &  2.0& 14.23 $\pm$ 0.11&	 7.032 $\pm$ 0.364&	0.50\\
   10 & $-$2.0& 14.36 $\pm$ 0.12&	 7.444 $\pm$ 0.421&	0.55\\
   17 & $-$2.0& 13.87 $\pm$ 0.15&	 5.947 $\pm$ 0.441&	1.01\\
   1 &  5.0& 14.57 $\pm$ 0.12& 	 8.214 $\pm$ 0.444&	0.45\\
   3 &  5.0& 14.28 $\pm$ 0.12& 	 7.185 $\pm$ 0.414&	0.46\\
   3 & $-$5.0& 14.35 $\pm$ 0.12& 	 7.411 $\pm$ 0.390&	0.47\\
   5 &  5.0& 14.16 $\pm$ 0.12& 	 6.785 $\pm$ 0.371&	0.43\\
   7 &  5.0& 14.04 $\pm$ 0.09& 	 6.430 $\pm$ 0.271&	0.72\\
\hline
  $-$5 &  5.0& 14.67 $\pm$ 0.11&     8.588 $\pm$ 0.459&	    0.43\\
  $-$3 &  5.0& 14.52 $\pm$ 0.09&     8.015 $\pm$ 0.340&	    0.49\\
  $-$2 &  5.0& 14.56 $\pm$ 0.14&     8.183 $\pm$ 0.502&	    0.48\\
   0 &  7.5& 14.35 $\pm$ 0.13&     7.416 $\pm$ 0.415&	    0.45\\
   5 & $-$3.5& 14.00 $\pm$ 0.16&     6.319 $\pm$ 0.431&	    0.42\\
   5 &  3.5& 13.72 $\pm$ 0.14&     5.549 $\pm$ 0.343&	    0.44\\
   5 &  7.5& 14.21 $\pm$ 0.14&     6.943 $\pm$ 0.524&	    0.50\\
   10 & 3.5& 13.84 $\pm$ 0.16&     5.855 $\pm$ 0.463&	    0.43\\
\hline
 \end{tabular}
\end{table}