\begin{table}%tA.1
\caption{\label{verywidebinaries.1}Basic data from the literature of Washington double stars with tabulated angular separations $\rho > 1000$~arcsec.} 
\small \begin{tabular}{lll cccc c ccc l cc}
\hline  \hline\noalign{\smallskip}
WDS& Discovery  	& Simbad		& $\alpha$	& $\delta$      & $\mu_\alpha \cos{\delta}$	& $\mu_\delta$  	& $d_\pi$		& $V^{b}$ 	& $J$ 			& $K_{\rm s}$ 		& Sp.	 	& $\rho$	& $\theta$      \\ 
identifier  	& designation$^{a}$& name		& (J2000)	& (J2000)       & [mas~a$^{-1}$]		& [mas~a$^{-1}$]	& [pc]  		& [mag]		& [mag]			& [mag]			& type		& [arcsec]	& [deg]	        \\ % &  		     & [km~s$^{-1}$]	   
            \noalign{\smallskip}
            \hline
            \noalign{\smallskip}
%%
00059+1805	& LEP   1AE	& \object{HD 101}	& 00 05 54.74	& +18 14 05.8 	& --$152.2\pm1.1$ & --$148.1 \pm 1.4$	& $37.1\pm0.8	$ 	& 7.46 		& $6.332\pm0.019$ 	& $6.034\pm0.024$ 	& F8		& 1606.8	& 245.9	        \\ % & No $d_{\rm phot}$     & --45.6$\pm$0.1	   
&		& \object{LP 404--21}	& 00 04 11.81	& +18 03 10.7	& --146				& --146			& ...		  	& 16.3		& $14.068\pm0.030$ 	& $13.339\pm0.029$ 	& ...		&		& 	        \\ % &  		     & ...		   
            \noalign{\smallskip}
00152+2454	& GIC   4	& \object{G 131--46}	& 00 16 53.59	& +24 20 48.7  	& --$136\pm11$ 			& --$204\pm10$ 		& ...		 	& 13.6		& $9.944\pm0.020$ 	& $9.067\pm0.017$ 	& K		& 2469.8	& 145.8         \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{G 130--59}	& 00 15 11.85	& +24 54 52.1	& --$105\pm11$ 			& --$215\pm11$ 		& ...		  	& 14.5		& $12.600\pm0.022$ 	& $11.951\pm0.022$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
00400--1533	& LDS	5286	& \object{LP 765--52}	& 00 37 29.44	& --15 45 52.3  & $+173\pm5	$       		& --$19\pm5$       	& ...		 	& 15.5 *	& $11.890\pm0.021$ 	& $11.038\pm0.023$ 	& ...		& 2274.9	& 71.5	        \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{LP 765--57}	& 00 39 59.21	& --15 34 07.9	& $+169\pm5	$       		& --$34\pm5$       	& ...		  	& 15.2 *	& $13.317\pm0.026$ 	& $12.746\pm0.035$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
00435+3351	& WEI  46AC	& \object{GJ 30}	& 00 43 32.90	& +33 50 41.3	& --$204.0\pm0.8	$       	& --$357.2\pm0.6$       & $20.6\pm0.4	$ 	& 8.73		& $6.592\pm0.018$ 	& $5.938\pm0.016$ 	& K8		& 1295.0	& 266.8	        \\ % & No $\mu$ 	     & ...		   
		&		& \object{BD+33 96}	& 00 41 49.11	& +33 51 54.8	& $+8.3\pm1.2	$       		& $+1.8\pm1.2$       	& ...		  	& 8.63		& $6.639\pm0.021$ 	& $5.966\pm0.018$ 	& K0		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
00520+2035	& GIC	16	& \object{G 69--27}	& 00 52 00.03	& +20 34 58.6	& $+176.5\pm1.8	$       	& --$107.4\pm1.5$       & $32\pm3	$ 	& 11.40		& $8.490\pm0.019$ 	& $7.628\pm0.020$ 	& ...		& 1614.0	& 56.1	        \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{G 69--29}	& 00 53 35.48	& +20 49 59.4	&   $+213\pm11		$       	&   --$132\pm11$       	& ...		  	& 13.9 *	& $10.095\pm0.021$ 	& $9.248\pm0.015$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
01024+0504	& WNO  50AC	& \object{HD 6101} AB	& 01 02 24.60	& +05 03 41.4	& $+323.3\pm1.2	$       	& $+226.0\pm1.2$       	& $21.1\pm0.5	$ 	& 8.16		& $6.199\pm0.019$ 	& $5.510\pm0.020$ 	& K2+...	& 1276.0	& 87.8	        \\ % & Genuine  	     & +19.7		   
		&		& \object{G~1--45} AB	& 01 03 49.94	& +05 04 30.7	&   $+317\pm8		$       	&   $+227\pm8$       	& $21.3\pm1.7		$& 14.10		& $13.504\pm0.024$ 	& $13.418\pm0.034$ 	& DA5		&		&	        \\ % &  		     & +61.0		   
           \noalign{\smallskip}
01163--3217	& LDS	1091	& \object{LP 883--336}	& 01 16 21.75	& --31 58 12.2	& $+408\pm5	$       		& --$1\pm5	$       	& ...		 	& 17.9 *	& $11.899\pm0.022$ 	& $11.001\pm0.023$ 	& ...		& 1151.0	& 186.0	        \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{LP 883--337}	& 01 16 12.35	& --32 17 17.0	& $+388\pm5	$       		& $+17\pm5	$       	& ...		  	& 18.0 *	& $13.884\pm0.026$ 	& $13.132\pm0.034$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
02255--0904	& GRV	1148	& \object{WD 0223--092}	& 02 25 30.96	& --09 04 14.9	& $+81\pm5	$       		& --$2\pm5	$       	& ...		 	& 19.5 *	& ...		 	& ...		 	& DA4.6		& 1272.1	& 228.2	        \\ % & Follow-up	     & +84$\pm$129		   
		&		& \object{WD 0221--095}	& 02 24 26.96	& --09 18 23.5	& $+85\pm4	$       		& --$0\pm4	$       	& ...		  	& 19.8 *	& ...		 	& ...		 	& DA5.8		&		&	        \\ % &  		     & $+177\pm60		$   
           \noalign{\smallskip}
02310+0823	& GIC	32	& \object{G 73--63}	& 02 31 03.28	& +08 22 55.1	& $+376.1\pm1.9	$       	& --$85.4\pm1.6	$& $33\pm3	$ 	& 10.90		& $8.356\pm0.023$ 	& $7.554\pm0.023$ 	& K4--7V:	& 3094.6	& 277.9	        \\ % & Follow-up	     & ...		   
		&		& \object{G 73--59}	& 02 27 36.68	& +08 29 58.8	& +350		       		& --63		       	& ...		  	& 16.1 *	& $11.271\pm0.026$ 	& $10.455\pm0.021$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
03162+5810	& LEP	13AC	& \object{GJ 130.1 A}	& 03 16 13.82	& +58 10 02.4 	& $+445.6\pm3.9	$       	& --$340.3\pm4.1$ 	& $14.4\pm0.7	$ 	& 10.53		& $7.344\pm0.020$ 	& $6.566\pm0.024$ 	& M2 		& 1164.1	& 197.6	        \\ % & Follow-up	     & ...		   
		&		& \object{G 246--30}	& 03 15 29.44 	& +57 51 33.0	& +467		       		& --237		       	& ...		  	& 15.5 *	& $11.121\pm0.024$ 	& $10.271\pm0.019$ 	& M:		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
03330+0306	& LDS 	3504	& \object{G 80--8}	& 03 32 59.02	& +03 06 08.0 	& +294.8			& --80.9		& ...		  	& 13.1 *	& $10.102\pm0.023$ 	& $9.281\pm0.023$ 	& ... 		& 429.5		& 266.4	        \\ % & $\rho <$ 1000~arcsec & ...		   
		&		& \object{NLTT 11184}	& 03 32 30.40 	& +03 05 40.8	& +286		       		& --77		       	& ...		  	& 17.0 *	& $12.491\pm0.026$ 	& $11.750\pm0.029$ 	& ...		&		&	        \\ % &  		     & ...		   
           \noalign{\smallskip}
03442--6448	& LDS 	104	& \object{$\beta$ Ret} AB& 03 44 11.96	& --64 48 24.9 	& $+310.1\pm0.7	$       	& $+83.2\pm0.6		$& $29.9\pm0.5	$ 	& 3.84		& $1.937\pm0.310$ 	& $1.279\pm0.270$ 	& K2III SB 	& 1466.3	& 94.2	        \\ % & No $d_\pi$	     & $+50.8\pm0.9		$  
		&		& \object{HD 24293}	& 03 48 01.12 	& --64 50 11.7	& $+334.0\pm1.0	$       	& $+99.0\pm1.1		$ & $40.5\pm1.3	$ 	& 7.85		& $6.630\pm0.029$ 	& $6.241\pm0.024$ 	& G3V		&		&	        \\ % &  		     & +20.8$\pm$0.3, +19.3$\pm$2.0		  
           \noalign{\smallskip}
07590--6338	& LDS 199	& \object{CD--63 370}	& 07 58 57.36	& --63 37 45.5	& --$143.0\pm1.7	$       	& $+262.5\pm1.8$        & ...	 		& 9.90		& $8.826\pm0.034$ 	& $8.502\pm0.023$ 	& F8		& 1033.4	& 195.8		\\ % 
		&		& \object{L 137--85}	& 07 58 14.99	& --63 54 19.6	& --$178\pm10		$       	& $+384\pm10$       	& ...		  	& 11.2 *	& $9.791\pm0.024$ 	& $9.175\pm0.023$ 	& ...		&		&	        \\ % 		   
           \noalign{\smallskip}
10197+1928	& WNO  53	& \object{40~Leo}	& 10 19 44.20	& +19 28 15.8	& --$230.0\pm0.9	$       	& --$214.7\pm0.5$       & $21.37\pm0.11	$& 4.78		& $4.037\pm0.292$ 	& $4.020\pm0.314$ 	& F6IV		& 5231.4	& 308.3		\\ % Vr=+6.8+/-0.9km/s
		&		& \object{LP~371--59} A & 10 14 53.94	& +20 22 18.9	& --225			       	& --198       		& ...		  	& 15.3 *	& $10.815\pm0.026$ 	& $9.99\pm0.023$ 	& M5		&		&	        \\ % 		   
           \noalign{\smallskip}
11125+3549	& STTA	108BD	& \object{HD 97371}	& 11 12 44.28	& +35 49 48.4 	& --$60.1\pm0.7	$       	& --$7.8\pm0.7		$ & $141\pm13	$ 	& 7.20		& $5.423\pm0.019$ 	& $4.805\pm0.018$ 	& K0	 	& 2100.8	& 88.5	        \\ % & No $\mu$ 	     & ...
		&		& \object{HD 97832}	& 11 15 36.98 	& +35 50 44.7	&   $+0.1\pm1.2$ 		& --2.2$\pm$1.3 		& ...		 	& 8.20		& $6.668\pm0.021$ 	& $6.194\pm0.018$ 	& G5		&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
11452+1821	& GIC	101	& \object{G 57--17}	& 11 45 11.92	& +18 20 58.7	& --$296\pm8$ 			& --$296\pm8$ 		& ...		 	& 13.27		& $9.162\pm0.022$ 	& $8.260\pm0.016$ 	& M4		& 1341.3	& 280.2	        \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{G 57--15}	& 11 43 39.18	& +18 24 56.9	& --259		       		& --267		       	& ...		  	& 15.07		& $12.863\pm0.026$ 	& $12.097\pm0.021$ 	& ...		&		&	        \\ 		     11455+4740	& LEP	45	& \object{HD 102158}	& 11 45 30.58	& +47 40 01.1	& --591.6~$\pm$~0.7	       	& 
--290.7~$\pm$~0.5	 & 49.3~$\pm$~1.7		& 8.06		& 6.860~$\pm$~0.026 	& 6.509~$\pm$~0.026 	& G2V		& 1176.1	& 72.4	        \\ 
		&		& \object{G 122--46}	& 11 47 21.66 	& +47 45 56.7	& --585		       		& --200		       	& ...		  	& 14.16		& 10.586~$\pm$~0.020 	& 9.846~$\pm$~0.020 	& M:		&		&	        \\ % &  		     & ... [V=14.16, R=13.00, I=11.96, d=48(2)pc]		   
           \noalign{\smallskip}
13090+3353	& LEP  62AC	& \object{LP 268--35}	& 13 08 58.26	& +33 53 10.0	& --209.7~$\pm$~2.3	      	& --111.8~$\pm$~1.7	& 66~$\pm$~12	 	& 11.56		& 9.296~$\pm$~0.019 	& 8.623~$\pm$~0.018 	& ...		& 1273.8	& 192.3	        \\ % & Follow-up	     & ...		   
		&		& \object{LP 268--33}	& 13 08 36.42 	& +33 32 25.7	& --208.8~$\pm$~5.5 		& --101.2$~\pm~$5.5 	& ...		  	& 16.3 *	& 11.685~$\pm$~0.021 	& 10.769~$\pm$~0.019 	& ...		&		&	        \\ % &  		     & ... 
           \noalign{\smallskip}
13410+6808	& LDS	5788	& \object{G 238--50}	& 13 44 29.36 	& +68 27 50.3	& --269.9~$\pm$~1.5	      	& 
+43.5~$\pm$~1.8 		& 40~$\pm$~3		& 11.17		& 8.845~$\pm$~0.021 	& 8.023~$\pm$~0.015 	& M2		& 1696.8	& 44.5	        \\ % & No $d_{\rm phot}$     & ...		   
		&		& \object{LP 40--200}	& 13 40 54.27	& +68 07 43.8	& --265.5~$\pm$~1.8 		& 
		+32.8~$\pm$~1.8		& ...		  	& 11.83		& 9.837~$\pm$~0.019
		 	& 9.138~$\pm$~0.020 	& K3		&		&	        \\ % &  		     & ... 
           \noalign{\smallskip}
13599+2520	& BUP	156	& \object{BD+26 2517} AB& 14 01 11.60   & +25 21 36.2   & +5.5~$\pm$~1.4 			& +36.2~$\pm$~1.3	 	& ... 		  	& 9.51	  	& 8.337~$\pm$~0.023 	& 8.060~$\pm$~0.018 	& G0  	  	& 1033.9	& 83.2	        \\ % & No $\mu$ 	     & ... 
		&		& \object{BD+26 2513}	& 13 59 55.87   & +25 19 33.7   & $+20.5\pm1.2$ 			& --55.9~$\pm$~1.2 	& ... 		  	& 10.41	  	& 9.433~$\pm$~0.021 	& 9.145~$\pm$~0.019 	& F8  	  	&		&	        \\ % &  		     & ...		     
           \noalign{\smallskip}
14396--6050$^{c}$& LDS	494AC	& \object{$\alpha$ Cen} AB& 14 39 35.93 & --60 50 07.0 	& --3633.7~$\pm$~0.7 		& 
+702.3~$\pm$~0.6  	& 1.325~$\pm$~0.007 	& 1.35		& --1.454~$\pm$~0.133
 	& --2.008~$\pm$~0.260 	& G2V+K1V 	& 7860.1	& 236.9	        \\ % & Genuine  	     & $--$22.4\pm2.7/--22.4\pm1,1$$ G2V+K1V (Torres et al. 2006)
		&		& \object{Proxima}	& 14 29 42.91   & --62 40 46.5  & --3775.8~$\pm$~1.6 		& 
		+766~$\pm$~2	  	& 1.296~$\pm$~0.004 	& 11.01	  	& 5.357~$\pm$~0.023
		 	& 4.384~$\pm$~0.033 	& M5.5Ve  	&		&	        \\ % &  		     & --$22.4\pm0.5$ M6Ve (Torres et al. 2006) / --33.4 (Hawley et al. 1996)		     
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15208+3129	& LEP	74	& \object{HD 136654}	& 15 20 50.07  	& +31 28 48.5  	& --180.0~$\pm$~0.4 		&
 +139.0~$\pm$~0.5 	& 43.5~$\pm$~1.1 		& 6.90	  	& 5.982~$\pm$~0.020 	& 5.742~$\pm$~0.027 	& F5V	    	& 1580.6	& 325.6	        \\ % & Genuine  	     & --27.3$\pm$0.3, 2004A&A...418..989N
		&		& \object{BD+32 2572}	& 15 19 40.15   & +31 50 32.9  	& --181.2~$\pm$~0.6	
			& +140.2~$\pm$~0.8 	& 42~$\pm$~2 		& 9.03	  	& 7.569~$\pm$~0.021 	& 7.115~$\pm$~0.020 	& K0V	  	&		&	        \\ % &  		     & --26.6$\pm$0.4, 2001MNRAS.328...45M; --25.5$\pm$1.0,--26.$9\pm0.5,$ 2000A&AS..142..275S  		     
           \noalign{\smallskip}
16348--0412	& GIC	144AB	& \object{HD 149414} AB	& 16 34 42.36  	& --04 13 44.1  & --133.7~$\pm$~1.4 		&
 --701.2~$\pm$~1.4 	& 45~$\pm$~3 		& 9.60	  	& 8.055~$\pm$~0.024 	& 
 7.517~$\pm$~0.024 	& G5Ve SB$_1$	& 1176.5	& 36.4	        \\ % & Follow-up	     & --171.29$\pm$1.93, 2002AJ....124.1144L [Moderate H and K emission, Cowley et al. 1967] [Metal-poor, [Fe/H] ~ -1.4] [SB1 M1=0.92 Msol, M2=0.52 Msol (DM91, Mazeh et al. 1997)]
		&		& \object{BD--03 3968B}	& 16 35 29.03 	& --03 57 57.2  & --162				& --685			& ... 		  	& 13.86	  	& 11.086~$\pm$~0.022 	& 10.541~$\pm$~0.022
		 	& M:	  	&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
18111+3241	& LEP	87	& \object{BD+32 3065}	& 18 11 06.22  	& +32 41 00.3	& --134.7~$\pm$~1.2
 		& +322.1~$\pm$~1.3 	& 46~$\pm$~3		& 10.52	  	& 8.590~$\pm$~0.039	
		& 7.931~$\pm$~0.020	& K5		& 1106.0	& 148.3	        \\ % & Follow-up	     & ...
		&		& \object{G 206--16}	& 18 11 52.28 	& +32 25 20.0  	& --143				& +318			& ... 		  	& 15.6 *	& 10.885~$\pm$~0.021	
		& 10.024~$\pm$~0.017	& ...	  	&		&	        \\ % &  		     & ...
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20084+1503	& LDS	1033AF	& \object{G 143--33}	& 20 08 21.93  	& +15 02 36.6	& --159.1~$\pm$~1.7		& --180.7~$\pm$~1.7	& ...			& 11.56	  	& 9.408~$\pm$~0.028	& 8.409~$\pm$~0.024	& ...		& 2186.6	& 269.0	        \\ % & No $d_{\rm phot}$     & ...
		&		& \object{G 143--27}	& 20 05 51.01 	& +15 01 59.2  	& --156				& --210			& ... 		  	& 12.88		& 11.626~$\pm$~0.022	& 11.245~$\pm$~0.020	& ...	  	&		&	        \\ % &  		     & --$22.43\pm0.41,$ 2002AJ....124.1144L
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20124--1237	& TDT	2085AC	& \object{$\xi^{02}$ Cap}& 20 12 25.86  	& --12 37 02.5	&+193.4~$\pm$~0.4		& --196.0~$\pm$~0.5	& 27.7~$\pm$~0.3		& 5.84	  	& 4.971~$\pm$~0.020	& 4.634~$\pm$~0.017	& F7V		& 1021.3	& 193.6	        \\ % & Genuine  	     & $+27.1\pm1.3,$ 2004A&A...418..989N
		&		& \object{LP 754--50}	& 20 12 09.44 	& --12 53 35.1  & +195.3~$\pm$~2.0		& --194.8~$\pm$~1.8	& 23.6~$\pm$~1.4		& 11.30		& 8.485~$\pm$~0.023	
		& 7.625~$\pm$~0.021	& M0Vk	  	&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
20302+2651	& BUP	213AE	& \object{HD 340345} AB	& 20 30 10.67  	& +26 50 34.5	& --145.9~$\pm$~2.7		& --141.9~$\pm$~2.7	& 23.8~$\pm$~1.8		& 9.69	  	& 7.133~$\pm$~0.021	
& 6.347~$\pm$~0.020	& M1V+		& 1338.7	& 93.2	        \\ % & No $\mu$ 	     & $+17.8\pm5.0,$ 1979IAUS...30...57E
		&		& \object{HD 340459}	& 20 31 50.53 	& +26 49 19.3  	& --8.1~$\pm$~1.4			& --5.5~$\pm$~1.4		& ... 		  	& 10.15		& 8.235~$\pm$~0.023	
		& 7.647~$\pm$~0.016	& G5	  	&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
20452--3120	& LDS	720AB	& \object{AU Mic}	& 20 45 09.49  	& --31 20 26.7	& +279.6~$\pm$~1.2		& --360.3~$\pm$~0.8	& 9.92~$\pm$~0.10		& 8.81	  	& 5.436~$\pm$~0.017	
& 4.529~$\pm$~0.020	& M1Ve		& 4680.9	& 212.8	        \\ % & Genuine  	     & --$3.3\pm2.0$
		&		& \object{AT Mic} AB	& 20 41 51.12 	& --32 26 07.3  & +261.3~$\pm$~3.6		& --344.8~$\pm$~3.9	& 10.7~$\pm$~0.4		& 10.27		& 5.807~$\pm$~0.026	& 
		4.944~$\pm$~0.042	& M4Ve+M5:	&		&	        \\ % &  		     & --$3.7\pm3.0$
           \noalign{\smallskip}
20599+4016	& LEP  98AD	& \object{HD 200077} AE--D& 20 59 55.24	& +40 15 31.4	& +230.5~$\pm$~01.1		
& +211.2~$\pm$~1.3	& 41.0~$\pm$~0.9		& 6.58	  	& 5.450~$\pm$~0.021	& 5.119~$\pm$~0.024	& F8+		& 1212.8	& 258.5	        \\ % & Genuine  	     & --$36.1\pm1.0,$ 2004A&A...418..989N
		&		& \object{G 210--44} AB	& 20 58 11.48 	& +40 11 29.0   & +229.7~$\pm$~1.2		& +202.9~$\pm$~1.2	& 46~$\pm$~4		& 10.75		& 8.142~$\pm$~0.030	& 7.339~$\pm$~0.018	& M1		&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
22175+2335	& GIC 	179	& \object{G 127--13}	& 22 17 25.87  	& +23 35 04.7	& --104~$\pm$~12			&
 --388~$\pm$~11		& ... 		  	& 14.1 *	& 9.890~$\pm$~0.019	& 9.057~$\pm$~0.023	& ...	
 	& 2107.7	& 12.7	        \\ % & Follow-up ???	     & ...
		&		& \object{G 127--14}	& 22 17 59.56 	& +24 09 21.1   &
		 --124~$\pm$~10			& --416~$\pm$~10		& ... 		  	& 14.2 *	& 10.276~$\pm$~0.021	& 9.49~$\pm$~0.018	& ...		&		&	        \\ % &  		     & ...
           \noalign{\smallskip}
23228+2208	& GIC 	191	& \object{BD+21 4923} 	& 23 22 48.81  	& +22 07 59.4	& +198.3~$\pm$~1.2		& --69.8~$\pm$~1.2	& 71~$\pm$~9		& 9.71		& 8.293~$\pm$~0.020	& 7.851~$\pm$~0.016	& F5		& 3265.3	& 253.9	        \\ % & No $\mu$ 	     & ...
		&		& \object{G 68--7}	& 23 19 03.21 	& +21 52 54.5   &   +310~$\pm$~11			&  --101~$\pm$~11		& ... 		  	& 14.7 *	& 11.589~$\pm$~0.020	& 10.784~$\pm$~0.018	& ...		&		&	        \\ 
\hline
\end{tabular}
\begin{list}{}{}
\item[$^{a}$] References of discovery names -- BUP: Burnham, S.~W. proper motion stars (from additional ``DD'' list): GIC: Giclas et~al. (\cite{Gi61}); 
GRV: Greaves, J. private communication (from data in Eisenstein et~al. \cite{Ei06}); LEP: L\'epine \& Bongiorno (\cite{LaB07});  LDS: Luyten, W.~J. proper motion catalogues (e.g. Luyten \cite{Lu41});  
STF: Struve, F.~J.~W. (several citations by e.g.: Herschel \cite{He1833}; Bessel \cite{Be1833}); STTA: Struve, O. ``DD'' (Appendix list);
TDT: Tycho Double Star (from additional ``DD'' list); WNO: Washington Observations; WEI: Weisse, M. (cited in, e.g., Burnham Double Star Catalogue~1906).  \item[$^{b}$]~$V$-band magnitudes marked with  an asterisk are estimated from  four epochs of photographic $B_J$ and $R_F$ magnitudes or from Sloan $g$ and $r$ magnitudes. Remaining $V$-band magnitudes are from the literature (see main text). \item[$^{c}$] The proper motion of the primary in the system corresponds to $\alpha$~Cen~A. The apparent difference with respect Proxima (of up to $292 \pm 4$~mas~a$^{-1}$ in $\mu_\delta$) is due to the strong dynamical effect on $\alpha$~Cen~A by its close companion, $\alpha$~Cen~B. 
\end{list}
\end{table}