\begin{table}%ta2
\par
\caption{\label{tabB}Results: $V_{\rm rad}$, $V_{\rm rot}$, Li equivalent width, Li abundance, Binarity.}
\small%\centerline
{
\begin{tabular}{rrrcccccc}
 \hline\hline\noalign{\smallskip}
    \noalign{\smallskip}
    nep    &  $V_{\rm rad}$ (km s$^{-1}$)   &    $V_{\rm rot}$ (km s$^{-1}$)	&     $EW_{\rm Li}$(m\AA)  &   $T_{\rm eff}$(K) &$N_{\rm Li}$ & $N_{\rm Li}$$^{\rm NLTE}$ &Spectral type &notes \\ \noalign{\smallskip}\hline
  $^*$20       &  --17.3~$\pm$~0.9  & $\le$3.5      &$<$4.3   & 5310~$\pm$~150	 & $<$0.68        &$<$0.77	      &  G8  &\\
 260        &  --19.5~$\pm$~1.1  & 11.1~$\pm$~2.1  &112.4     & 5790~$\pm$~150		&2.76~$\pm$~0.24	   &2.71~$\pm$~0.19   & G2&\\	
 330        &  --35.4~$\pm$~1.0  & 6.7~$\pm$~0.8   &$<$3.6   & 5250~$\pm$~150	 &$<$0.53	    	&		& G9&\\
 370        &  --15.7~$\pm$~1.3  & 7.0~$\pm$~1.0   &119.3     & 6250~$\pm$~300		&3.22~$\pm$~0.28     &3.09~$\pm$~0.20	& F8&\\
$^*$1420       &                 & 22.7~$\pm$~1.0  &--        & 5150~$\pm$~150		&  		  	&		&K0&\\
$^*$1441       &  --15.7~$\pm$~1.5  & 4.0~$\pm$~1.4   &56.2      & 5790~$\pm$~150		&2.34~$\pm$~0.20	   &2.34~$\pm$~0.18	& G2&\\
1470        &  --10.2~$\pm$~1.0  & 7.4~$\pm$~0.4   &106.2     & 5310~$\pm$~150		& 2.22~$\pm$~0.24	   & 2.27~$\pm$~0.21	& G8&\\
1500        &  --17.0~$\pm$~0.8  & 5.5~$\pm$~0.7   &10.7      & 5790~$\pm$~150		&1.57~$\pm$~0.18     &1.59~$\pm$~0.18	& G2&\\
1511        &                 &              &87.0      & 4450~$\pm$~350		&1.01~$\pm$~0.50    	&		& K4 (?)&x\\
1580        &                 &              &65.1      & 4830~$\pm$~300		& 1.36~$\pm$~0.40   & 1.55~$\pm$~0.37	& K2 (?)&x\\
$^*$1600       &  --18.8~$\pm$~0.9  & 5.4~$\pm$~1.4   &--        & 5790~$\pm$~150		& 		   	&		& G2&\\
1601        &  --13.0~$\pm$~1.4  & 11.0~$\pm$~0.7  &135.6     & 5940~$\pm$~150		& 3.05~$\pm$~0.24    & 2.94~$\pm$~0.18	&G0&\\
1690        &  --37.0~$\pm$~2.7  & 10.1~$\pm$~1.0  &--        & 5790~$\pm$~150		&  		   	&		&G2&\\
1800        &  --58.0~$\pm$~4.1  & 16.3~$\pm$~1.4  &98.1      & 6650~$\pm$~300		& 3.28~$\pm$~0.22	   & 3.16~$\pm$~0.18	 &F5&\\
1840        &                 &    $\ge$30.0           &--        & 5940~$\pm$~150		&  		  	&		 &G0&\\
1960        &                 & $\ge$50.0     &--        & 7000~$\pm$~300		 &  		   	&		&F2&\\
2050        &  --7.6~$\pm$~1.8   & 12.8~$\pm$~1.0  &77.2      & 5150~$\pm$~150		 & 1.85~$\pm$~0.23   & 1.96~$\pm$~0.21	& K0&\\
2100        &                 &              &--        & 3500~$\pm$~350		&  		   	&		&M3&\\
2210        &  --7.1~$\pm$~1.8   & 25.0~$\pm$~2.0  &--        & 6250~$\pm$~300		 & 		    	&		& F8 (?)&x\\
2250        &  --7.4~$\pm$~0.9   & 3.8~$\pm$~0.7   &$<$3.0   & 5150~$\pm$~150	  &$<$0.33 	      	&		& K0&\\
2360        &  --26.2~$\pm$~1.4  & 8.2~$\pm$~0.7   &44.9      & 6250~$\pm$~300		 & 2.63~$\pm$~0.23   & 2.58~$\pm$~0.16	&F8&\\
2400        &  --14.3~$\pm$~0.9  & 4.5~$\pm$~1.4   &$<$3.9   & 5790~$\pm$~150	  &	$<$1.12    &	$<$1.16 	& G2&\\
2470        &                 & 8.3~$\pm$~1.0   &--       & 6950~$\pm$~300		 &  		    	&		& F3&\\
2480        &                 & $\ge$40.0             &--        & 5150~$\pm$~150		 & 		    	&		& K0&\\
$^*$2970       &                 & $\ge$60.0     &--        & 7000~$\pm$~300		 & 		    	&		& F2 (?)&x\\
$^*$3080       &  --12.9~$\pm$~1.7  & 20.6~$\pm$~1.0  &147.6     & 4800~$\pm$~350		 & 1.85~$\pm$~0.49   & 2.00~$\pm$~0.53	& K2.5 (?)&x\\
3220        &  --25.1~$\pm$~1.0  & $\le$3.5      &$<$5.4   & 5150~$\pm$~150	  & $<$0.60         	&$<$0.72		&K0&\\
3560        &  --2.6~$\pm$~1.3   & 7.9~$\pm$~1.0   &124.9     & 5310~$\pm$~150		 &  2.34~$\pm$~0.25  &  2.38~$\pm$~0.24	& G8&\\
3610        &  +9.7~$\pm$~1.0   & 5.1~$\pm$~0.7   &13.9      & 4450~$\pm$~400		 &   0.11~$\pm$~0.56   	&		&K4&\\
3690        &                 &              &--        &  9000~$\pm$~800 	&		    	&		&A2&\\
3710        &                 &$\ge$30.0      &--        & 7000~$\pm$~300 	 &		     	&		&F2&\\
$^*$4090       &  --40.7~$\pm$~2.2  & $\le$3.5      &--        & 5790~$\pm$~150 	 & 		     	&		&G2&\\
4100        &  +10.0~$\pm$~0.9  & 4.5~$\pm$~0.7   &18.2      & 5150~$\pm$~150		 & 1.14~$\pm$~0.18    & 1.27~$\pm$~0.31	 &K0&\\
4130        &                 &$\ge$40.0      &--        & 6650~$\pm$~300		 &  		     	&		&F5&\\
4180        &  --13.6~$\pm$~1.0  & $\le$3.5      &$<$3.0   & 5150~$\pm$~150	  & $<$0.33 		&		&K0&\\
4380        &  --21.8~$\pm$~1.1  & 6.3~$\pm$~1.4   &29.0     &   5560~$\pm$~200         & 1.81~$\pm$~0.24    & 1.86~$\pm$~0.23	&G5&\\
4470        &  --13.5~$\pm$~0.8  & 5.3~$\pm$~0.8   &24.3     & 4800~$\pm$~350		 & 0.85~$\pm$~0.45    & 1.06~$\pm$~0.44	 &K3&\\
4530        &  --21.6~$\pm$~1.8  & 14.2~$\pm$~0.7  &228.7    & 5300~$\pm$~150		 & 2.97~$\pm$~0.40    & 2.84~$\pm$~0.26	&G9&\\
4780        &  --26.3~$\pm$~2.1  & 11.7~$\pm$~1.1  &422.3    & 4830~$\pm$~300		 &  3.60~$\pm$~0.75   &  3.40~$\pm$~0.65	& K2&\\
4810        &  --37.0~$\pm$~1.6  & 7.8~$\pm$~1.0   &--       & 6650~$\pm$~300		 & 		      	&		& F5&\\
$^*$4931       &  +2.5~$\pm$~1.7   & 3.6~$\pm$~1.0   &$<$5.5  & 4000~$\pm$~150		  & $<$-0.8		&		& K8&\\
4970        &  +14.3~$\pm$~0.9  & $\le$3.5      &$<$8.6  & 4830~$\pm$~300		  &$<$0.41 		&		& K2&\\
5060        &  --2.3~$\pm$~0.9   & 7.6~$\pm$~2.1   &97.9     & 5560~$\pm$~200		 & 2.44~$\pm$~0.26    & 2.45~$\pm$~0.22	&G5&\\
5220        &  --18.9~$\pm$~2.0  & 25.8~$\pm$~2.2  &$<$4.8  & 6250~$\pm$~300 	  &$<$1.61 		&$<$1.59 	&F8&\\
$^*$5320       &  --19.4~$\pm$~0.8  & 4.0~$\pm$~0.7   &38.5     & 5150~$\pm$~150		 & 1.49~$\pm$~0.21     & 1.62~$\pm$~0.20	&K0&\\
5510        &  --53.5~$\pm$~3.0  & 20.4~$\pm$~2.1  &371.3    & 5150~$\pm$~150		 & 3.79~$\pm$~0.67     & 3.46~$\pm$~0.54	&K0 (?)&x\\
5520${^a}$  &   +8.0~$\pm$~1.3    & 7.6~$\pm$~1.0   &93.2     & 4450~$\pm$~350		  & 1.05~$\pm$~0.51	&		& K4 (?)&SB2\\
5520${^b}$  &   +25.7~$\pm$~2.3   & 4.2~$\pm$~1.4   &39.8     & 4450~$\pm$~350		  & 0.60~$\pm$~0.49	&		& K4 (?)&\\
5950        &  --20.6~$\pm$~1.4  & 11.4~$\pm$~1.0  &$<$4.3  & 5940~$\pm$~150		   & $<$1.30 		& $<$1.31	&G0&\\
6030        &  --13.2~$\pm$~1.0  & 4.5~$\pm$~1.4   &$<$5.0  & 4780~$\pm$~350		   &$<$0.11  		&		&K3&\\
6051        &  --9.1~$\pm$~1.3   & 15.1~$\pm$~1.0  &--       & 4410~$\pm$~400		  &  			&		&K5&\\
6160        &                                &  &--    & 7300~$\pm$~300		 & 			&		& F0&\\
6163        &  --7.4~$\pm$~0.5   & 3.7~$\pm$~1.4   &49.4     & 5700~$\pm$~150		  &2.19~$\pm$~0.19	&2.21~$\pm$~0.18	&G3&\\
6350        &                 & $\le$3.5      &--       & 3500~$\pm$~350		  &  			&		&M3&\\
6400        &  --23.9~$\pm$~0.8  & $\le$3.5      &$<$5.0  & 4830~$\pm$~300		   & $<$0.17		  &		& K2&\\
6410        &  --25.6~$\pm$~1.2  & $\le$3.5      &10.5     & 5150~$\pm$~150		  &0.89~$\pm$~0.21 	&1.02~$\pm$~0.21 	& K0&\\
6510        &                 &              &--       & 7300~$\pm$~300		 & 		        &		& F0&\\\hline
\end{tabular}}
\smallskip
Note: an x in column eight indicates that the star is (or it is supposed to be) binary. We indicate SB2 for double-lined spectroscopic
binary.\\
$^*$ We lack the thorium-argon lamp exposures for the nights in which these~stars were acquired. They
were wavelength calibrated using lamp exposures of the nearest night.\\
${^a}$ Primary and ${^b}$ secondary component of nep~5520 SB2 system. 
\end{table}