\begin{table}%t2
\caption{\label{tab2}Polarization results of stars in direction to NGC 5617.}
%\centering
\par
\begin{tabular}{lccccccc}
\hline \hline
\noalign{\smallskip}
Star\tablefootmark{a} & Other ids.\tablefootmark{b} & $P_{\rm max} \pm \epsilon_{p} $ & $\sigma_1$\tablefootmark{c} &
                $\lambda_{\rm max} \pm \epsilon_{\lambda}$ &  kin.~memb.\tablefootmark{d}
		 & this work \\
& & $ \%$&  & $\mu$m &      \\
\hline
36  &L96  &  3.31 $\pm$   0.10&  0.63&  0.63 $\pm$   0.05&             &  nm \\ 
55  &L180, RG &  2.36  $\pm$   0.22&  1.04&  0.49 $\pm$   0.07& nm(M; FM)    &  nm  \\ 
65  &L98  &  1.87  $\pm$   0.19&  1.25&  0.72 $\pm$   0.20&             &  nm \\         
68\tablefootmark{*} &L105, BS &  4.26  $\pm$   0.08&  0.78&  0.61 $\pm$   0.03&            & member \\  
79  &L46  &  4.93  $\pm$   0.39&  1.61&  0.70 $\pm$   0.12&            &   member \\ 
80  &L158 &  4.61  $\pm$   0.08&  0.29&  0.57 $\pm$   0.02&             &     nm \\  
93  &L94  &  4.60  $\pm$   0.22&  1.02&  0.54 $\pm$   0.06&            &  member \\  
94  &L45  &  4.37  $\pm$   0.10&  0.59&  0.50 $\pm$   0.02&            &   member \\         
100  &L47  &  5.05  $\pm$   0.29&  1.00&  0.43 $\pm$   0.03&            &   member \\ 
106  &L91  &  4.56  $\pm$   0.17&  0.71&  0.49 $\pm$   0.04&            &  member \\             
107  &L48  &  4.50  $\pm$   0.22&  1.32&  0.55 $\pm$   0.06&            &   member \\   
116\tablefootmark{*} &L42  &  4.13  $\pm$   0.03&  1.37&  0.55 $\pm$   0.01&  m(M; FM)  &  member \\ 
136  &L89  &  3.91  $\pm$   0.23&  1.80&  0.61 $\pm$   0.11&            &    nm    \\          
139  &L39  &  4.36  $\pm$   0.17&  1.10&  0.52 $\pm$    0.05&           &  member \\         
143  &L51  &  3.36  $\pm$   0.33&  1.78&  0.55 $\pm$   0.13&            &     nm  \\           
146  &L49  &  4.33  $\pm$   0.29&  1.84&  0.58 $\pm$   0.08&            &   member \\  
154  &L52  &  2.49  $\pm$   0.27&  3.47&  0.57 $\pm$   0.13&            &     nm  \\           
169  &L53  &  4.61  $\pm$   0.15&  0.92&  0.49 $\pm$   0.03&            &   member \\  
175  &L15  &  4.31  $\pm$   0.06&  0.48&  0.56 $\pm$    0.02&        &  member \\  
176 &L114 &  2.57  $\pm$   0.09&  0.55&  0.51 $\pm$   0.03&             &   nm   \\         
180  &L54  &  4.77  $\pm$   0.05&  0.47&  0.53 $\pm$   0.01&  m(FM)     &   member \\ 
182  &L86, BS  &  4.18  $\pm$   0.18&  0.87&  0.46 $\pm$   0.03&            &  poss.member\\  
184  &L87  &  4.76  $\pm$   0.14&  0.95&  0.53 $\pm$   0.04&            &  member \\      
185\tablefootmark{*} &L31, BS  &  4.43  $\pm$   0.03&  0.32&  0.52 $\pm$   0.01&           &  member \\
186 &L115 &  4.75  $\pm$   0.07&  0.43&  0.56 $\pm$   0.02&             &  member \\     
187\tablefootmark{*} &L2   &  1.83  $\pm$   0.26&  1.52&  0.63 $\pm$   0.20&        &  nm   \\
188  &L85  &  4.57  $\pm$   0.30&  1.04&  0.65 $\pm$   0.10&            &   member \\     
190  &L16  &  4.07  $\pm$   0.09&  0.83&  0.55 $\pm$    0.03&        &  member \\  
195\tablefootmark{*} &L1, BS   &  4.42  $\pm$   0.62&  2.21&  0.44 $\pm$   0.09&        &  poss. member\\
196  &L55  &  2.80  $\pm$   0.28&  1.39&  0.45 $\pm$   0.10&            &     nm     \\  
202\tablefootmark{*} &L29, BS  &  4.83  $\pm$   0.10&  1.33&  0.50 $\pm$   0.02&  nm(FM)   &  member \\  
203  &L56  &  4.53  $\pm$   0.11&  0.65&  0.52 $\pm$   0.02&            &   member \\  
205\tablefootmark{*} &L3   &  4.51  $\pm$   0.30&  0.93&  0.44 $\pm$   0.05&        &  member \\        
207\tablefootmark{*} &L4   &  3.69  $\pm$   0.16&  1.01&  0.52 $\pm$   0.05&        &  member \\ 
214 &L116 &  4.23  $\pm$   0.07&  0.59&  0.60 $\pm$   0.02&             &  member \\  
215  &L84  &  3.46  $\pm$   0.11&  0.98&  0.56 $\pm$   0.04&            & poss.member  \\          
216\tablefootmark{*} &L5   &  4.33  $\pm$   0.06&  0.51&  0.57 $\pm$   0.02&        &  member \\  
221  &L57  &  3.72  $\pm$   0.11&  0.95&  0.49 $\pm$   0.03&            &   member \\  
225\tablefootmark{*} &L28  &  4.82  $\pm$   0.17&  0.94&  0.51 $\pm$   0.03&           &  member \\         
226\tablefootmark{*} &L26  &  4.16  $\pm$   0.48&  1.91&  0.70 $\pm$   0.22&           &  member  \\        
227\tablefootmark{*} &L17, RG  &  4.38  $\pm$   0.18&  2.29&  0.48 $\pm$   0.03&  m(M; FM)& member \\         
238  &L59  &  3.95  $\pm$   0.45&  1.48&  0.55 $\pm$   0.13&            &   member \\         
244  &L23  &  3.86  $\pm$   0.12&  0.66&  0.55 $\pm$    0.04&           &  member \\                     258\tablefootmark{*} &L81  &  4.01  $\pm$   0.17&  1.69&  0.54 $\pm$  0.05&            &   member \\ 
259 &L119 &  4.02  $\pm$   0.42&  1.06&  0.45 $\pm$   0.06&             &  member \\    
260 &L118 &  3.20  $\pm$   0.30&  2.26&  0.56  $\pm$   0.14&             & member  \\             261  &L20, BS  &  3.98  $\pm$   0.14&  2.32&  0.55  $\pm$    0.04&        &  poss.member \\
269 &L120 &  3.46 $\pm$   0.11&  0.59&  0.58 $\pm$   0.05&             &   nm \\    
270 & L82  &  4.31 $\pm$   0.26&  2.36&  0.49 $\pm$   0.05&            & poss.member  \\      
274 & L62  &  4.19 $\pm$   0.39&  2.39&  0.59 $\pm$   0.13&            &   member \\         
275 & L61  &  4.09 $\pm$   0.57&  1.58&  0.47 $\pm$   0.11&            &   member \\        
276 & L68  &  4.71 $\pm$   0.05&  0.24&  0.60 $\pm$   0.01&            &   member \\        
379 & L64  &  3.25 $\pm$   0.15&  1.11&  0.57 $\pm$   0.07&            &     nm   \\            
292 & L65  &  4.30 $\pm$   0.37&  1.67&  0.43 $\pm$   0.05&            &   member \\        
294 & L66  &  3.90 $\pm$   0.18&  0.80&  0.48 $\pm$   0.04&            &   member \\       
295 &L121 &  3.78 $\pm$   0.10&  0.54&  0.58 $\pm$   0.05&             &  member \\   
302 &L122 &  4.35 $\pm$   0.11&  0.75&  0.65 $\pm$   0.04&             &  member \\  
321 &L143 &  2.31 $\pm$   0.29&  0.69&  0.42 $\pm$   0.08&             &     nm          \\     
327 &L144 &  3.05 $\pm$   0.21&  1.55&  0.56 $\pm$   0.08&             &     nm          \\  
330 &L141 &  4.29 $\pm$   0.13&  1.94&  0.57 $\pm$   0.04&             &  member  \\ 
331 &L123 &  3.30 $\pm$   0.18&  1.30&  0.66 $\pm$   0.11&             &  nm  \\  
333 &L129 &  5.32 $\pm$   0.40&  1.88&  0.62 $\pm$   0.13&             &  nm          \\     
334 &L138 &  4.64 $\pm$   0.16&  1.31&  0.52 $\pm$   0.05&             &  member  \\ 
336 &L142 &  3.73 $\pm$   0.53&  1.75&  0.71 $\pm$   0.19&             &     nm         \\     
339\tablefootmark{*} &L124 &  3.92 $\pm$   0.20&  1.08&  0.55 $\pm$   0.06&            &  nm \\  
342 &L126 &  3.08 $\pm$   0.07&  0.79&  0.63 $\pm$   0.04& nm(M; FM)    &  nm         \\  
347 &L125 &  2.12 $\pm$   0.13&  1.39&  0.60 $\pm$   0.09&  nm(M; FM)   &  nm   \\     
\hline
\end{tabular}
\tablefoot {
\tablefoottext{a}{Identifications from Haug (\cite{H78});}
\tablefoottext{b}{identifications from Lindoff (\cite{L68}); RG: Red giant, BS: Blue straggler;}
\tablefoottext{*}{membership according to photometric studies;}
\tablefoottext{c}{${\sigma_{1}}^{2} = \sum {(r_{\lambda}/{\epsilon_{p_\lambda}})^2}/(m-2)$; where
$m$~is the number of colors and $r_{\lambda} = P_{\lambda} - P_{\rm
max}~\exp(-K~{\rm ln}^2({\lambda_{\rm max}/{\lambda}))}$;}
\tablefoottext{d}{membership according to Mermilliod et~al. (M) (\cite{MMU08}) and/or Frinchaboy
\& Majewski (FM) (\cite{FM08}).}}
\end{table}