\begin{table}%t2
%\centering
\par
\caption{Diffuse interstellar bands investigated in this study. 
  Equivalent widths ({\it EW}) and associated statistical errors $\sigma_{\it EW}$ are quoted in m\AA. 
  For non-detected DIBs upper limits are given; 
  {\it EW}$_{\rm upper\ limit}  = 3  \times \sigma_{\rm continuum} \times {\it FWHM}_{\rm DIB}$,
  with $\sigma_{\rm continuum}$ the noise on the adjacent continuum, and {\it FWHM}$_{\rm DIB}$ the expected full width at
  half maximum of the respective DIB.
  The \Ebv\ values were derived by subtracting the Milky Way foreground contamination from the line of sight reddening 
  (see Sect.~\ref{sec:Ebv} and Tables~\ref{tb:obs} and~\ref{tb:Ebv}). 
  The "$\times$'' signifies DIBs that were not covered by the spectral setting, and the (B) indicates possible blending with
  stellar or instrumental features.
  We have derived upper limits for DIB strengths towards the low reddened target \object{Sk~--67 5}.
  \mbox{\object{Sk~--70 120}} has been used as the reference star (\Ebv~=~0.0~mag). 	
\label{tb:EW_DIBs}}
%\resizebox{\columnwidth}{!}{
\begin{tabular}{llrrrrr}\hline\hline
	     && \multicolumn{5}{c}{LMC} \\\hline
	     && \multicolumn{1}{c}{\object{Sk --69 223}}  & \multicolumn{1}{c}{\object{Sk --69 243}}  &
 \multicolumn{1}{c}{\object{Sk~--67 2}} & \multicolumn{1}{c}{\object{Sk~--68 135}}& \multicolumn{1}{c}{\object{Sk~--67 5}} \\ 
\Ebv$_{\rm, LMC}$ && \multicolumn{1}{c}{0.20}  & \multicolumn{1}{c}{0.29}  &
 \multicolumn{1}{c}{0.12} & \multicolumn{1}{c}{0.14}& \multicolumn{1}{c}{0.04} \\ \hline
DIB	& $\lambda_{\rm LMC}$ & {\it EW} ($\sigma_{\it EW}$) & {\it EW} ($\sigma_{\it EW}$)  & {\it EW} ($\sigma_{\it EW}$)& {\it EW} ($\sigma_{\it EW}$) & {\it EW} ($\sigma_{\it EW}$)   \\ \hline%
4428	& 4431.95	      & $<$180 	   &	 150	 (180)  	 & $<$247		 &  $<$200	   &   $<$200        \\
5705	& 5710.23	      & 20	 (9)	   &	 25	 (21)		 & $<$32		 &  $<$23	   &   $<$28  (B)    \\
5780	& 5785.57	      & 145	 (2)	   &	$\times$			 & $\times$			 &  $\times$		   &	 $\times$	      \\
5797	& 5802.21	      & 28	 (6)	   &	$\times$			 &  $\times$			 &  $\times$		   &	 $\times$	      \\
5849	& 5855.08	      & $<$8		   &	 11	 (6)		 &     10     (5)	 &  5	       (5) &   $<$15	      \\
6196	& 6201.57	      & 12	 (3)	   &	 7	 (3)		 &     5      (3)	 &   $<$7	   &   $<$7	      \\
6203(B) & 6208.67	      & 50	 (20)	   &	 25	 (14)		 &     19     (14)	 &   17        (17)&   $<$17	      \\
6284    & 6289.51	      & 240	 (21)	   &	 335	 (47)		 &     150    (29)	 &	 30   (30) &   
$<$163        \\
6376	& 6381.71	      & 5	 (6)	   &	$<$28  		 & $<$23		 &  $<$20     (B) &   $<$17	      \\
6379	& 6384.96	      & 12	 (4)	   &	 15	 (4)		 & $<$10		 &  $<$10     (B) &   $<$7	      \\
6613	& 6619.51	      & 20	 (8)	   &	 50	 (14)		 &     13     (8)	 &  5	    (3) (B)&   $<$13	      \\
\hline
\end{tabular}
%}
\end{table}