01000+5702 MLR 626     Also known as TDS1710.                                                          
01000-7234 OGL 123     SMC105.4.9983  + SMC105.4.11297                                         Pli2012 
01001+4443 STF  79     164 And. Both A and B are spectroscopic binaries.                               
                       H N  45.                                                                MEv2010 
01001+1246 GWP 113     XMI 164.                                                                Tob2012b
01001-7135 OGL 124     SMC109.2.10029 + SMC109.2.10470                                         Pli2012 
01002+5809 SKF  56BC   Aka MRI  25.                                                                    
01005-1923 SHY 392     HIP   4702 + HIP   4833.                                                        
01006+6027 BAG  36     Primary is the alpha2 CVn type variable V551 Cas.                               
01006-7343 OGL 125     SMC107.4.12713 + SMC107.3.646                                           Pli2012 
01007-7250 OGL 126     SMC105.2.10999 + SMC105.2.12098                                         Pli2012 
01007-7328 OGL 127     SMC106.2.10337 + SMC106.2.11173                                         Pli2012 
01008-7400 OGL 128     SMC107.2.7090  + SMC107.2.7244                                          Pli2012 
01010-7154 OGL 129     SMC108.4.34907 + SMC108.4.34906                                         Pli2012 
01011-7119 OGL 130     SMC114.5.140   + SMC114.5.363                                           Pli2012 
01012+3704 BRT2585     ALI 254.  Also known as TDS1720.                                                
01012-5610 HJ 3412     B is CPD-56@199.                                                                
01013+1745 GWP 116     XMI 165.                                                                Tob2012b
01014+3535 COU 854     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.42 +/- 1.13, 2.60, and 1.10 Msun, respectively.             Mlk2012 
01014+1155 BU  867     Misidentified in BDS and ADS. Corrections by Baize and Couteau.                 
                       A premature orbit has been calculated.                                          
01014-7120 OGL 131     SMC114.5.22    + SMC114.5.226                                           Pli2012 
01014-7210 OGL 132     SMC113.7.22785 + SMC113.7.22807                                         Pli2012 
01015+6922 A  2901     1984.9965: This autocorrelogram was remeasured; the new results are             
                       listed in catalog.                                                              
01015+1024 GWP 117     XMI 166.                                                                Tob2012b
01016+5339 HJ 2008     01015+5339SMA  11                                                               
01016-1630 LDS9107     Old LDS6107.                                                                    
01017+4635 A   927     BRT  75                                                                         
01017+2518 HDS 134     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.80 +/- 0.47, 2.33, and 2.40 Msun, respectively.             Mlk2012 
01018-0652 LDS  33     NLTT 3377/3378                                                          Chm2004 
01019+1405 GRV 984     Typo in original WDS designation - entered as 01010+1405.                       
01020+0214 LDS3221     LDS5310.                                                                        
01020-7201 OGL 133     SMC113.6.22750 + SMC108.3.39755                                         Pli2012 
01020-7304 OGL 134     SMC106.4.40341 + SMC111.5.15843                                         Pli2012 
01021-1516 LDS9108     Old LDS6108.                                                                    
01023+8153 KNT   1     A is an Algol type eclipsing binary, U Cep, P =19.3d.  There is                 
                       circumstellar matter.                                                           
01023+1131 PLQ  11     LDS1085.                                                                        
01023+0552 A  2003     Close, 0.2" or under. Position angles show large changes. A premature           
                       orbit has been computed.                                                        
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.79 +/- 1.16, 2.45, and 1.05 Msun, respectively.             Mlk2012 
01024+0504 HDS 135     Mean motion indicates P ~ 80 yr, rho decreasing.                        Msn1999b
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 1.13 +/- 0.11, 1.39, and 1.35 Msun, respectively.  Mlk2012 
           WNO  50     AC: GJ 3071 + GJ 1027. CPM pair.                                        Mkr2008 
01025+0933 GWP 119     XMI 167.                                                                Tob2012b
01025-7353 OGL 135     SMC107.3.8839  + SMC112.6.180                                           Pli2012 
01026+6221 WNO  51     GJ 49 + GJ 51. CPM pair.                                                Mkr2008 
01027+0908 RAO  39     RoboAO finds 2 companions - Optical?  2MASS: B at 32.4" 145.3d, below   RAO2015 
                       the MS, optical? Tokovinin & Lepine (2012) miss AB but list an optical  Tok2012c
                       companion at 1733".                                                     Tok2014d
                       AB: A is SB2 with P = 26.2 days (Griffin & Suchkov 2003). The tertiary  Grf2003 
                       companion B at 2".8 did not move substantially in a year since its              
                       discovery by Riddle et al. (2015), but the PM of the main component A   RAO2015 
                       is small and the astrometry is not conclusive. B is located below the           
                       MS on the CMD, although still within the errors of its photometry.              
                       Considering the small field crowding, we count B as likely physical.    Rbr2015d
01028+3148 sig Psc     Combined spectroscopic/interferometric solution (Palomar Testbed        Knc2004 
                       Interferometer) by Konacki & Lane (2004), yielding distance = 112.9             
                       +/- 0.9 pc, masses 2.65 +/- 0.27 and 2.36 +/- 0.24 Msun, spectral               
                       types B9.5V, diameters 0.16 and 0.15 mas.                                       
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 8.19 +/- 0.87, 5.71, and 2.40 Msun, respectively.             Mlk2012 
01028+0049 LDS5311     Error in WDS designation - incorrect precession of Luyten coordinates?  Luy1984 
01029+4702 GIC  17     G172-034/G172-035. The A component is the variable star V359 And.               
                       NLTT 3437/3438                                                          Chm2004 
01029+4121 HJ 1064     39 And.                                                                         
01029+0753 OCC 480     eps Psc                                                                         
01030+4723 STT  21     A may be a spectroscopic binary.                                                
01030-0450 BUP  13     25 Cet.                                                                         
01031-7358 OGL 136     SMC112.7.5     + SMC112.7.92                                            Pli2012 
01032+7113 JNN 250     LHS 1182. Estimated age 1000-10000 Myr; masses 0.21 +/- 0.04 and 0.13           
                       +/- 0.02 Msun; a ~2.7 au.                                               Jnn2014 
01032+6032 MLB  43     This is a physical pair, with relative motion much smaller than the             
                       proper motions. Relative motion may be affected by a perturbation in            
                       the radial direction with a period of 25y.                              Kiy2012 
01032+2006 LDS 873     NLTT 3462/3463                                                          Chm2004 
01033-6006 HJ 3416     Spectrum F6/8III/IV.                                                            
01033-7123 OGL 137     SMC114.5.6465  + SMC114.6.10201                                         Pli2012 
01035+5019 STF  83     Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01035-0535 RST4162     J 1442.                                                                         
01036-5516 DLR   1     AB is a low-mass binary with masses 0.19 +/- 0.02 and 0.17 +/- 0.02             
                       Msun. At a distance of 47.2 +/- 3.1 pc the projected distance between           
                       the stars is 12au.  They are orbited by an L-type companion at 84au,            
                       which shares common proper motion.  The companion is either a 12-13             
                       Mjup planet (assuming an age of 20 Myr) or a 14-15 Mjup brown dwarf             
                       (for an age of 50 Myr).                                                 Dlr2013 
01036-7138 OGL 138     SMC114.7.13732 + SMC114.8.18665                                         Pli2012 
01037+4051 LDS3225     AB: Also known as GIC  18.                                                      
                       BC: NLTT 3481/3482                                                      Chm2004 
                       BC: Aside from the companion seen in the AstraLux images, there is an           
                       additional possible wide companion at 26" separation, as noted in the           
                       WDS. The wide components have very similar proper motions (e.g. Roser   Rsr2010 
                       et al. 2010), so actual companionship seems probable.                   Jnn2012 
           BWL   5     AD:  Colors and/or astrometry are inconsistent with a late-type common          
                       proper motion companion based on visual inspection of the field from            
                       2MASS, SDSS, DSS1, and/or DSS2. Primary is G 132-50.                    Bwl2015 
01037-3024 B   649     CI Scl, Algol (EA) type eclipsing binary, P = 14.7104 d.                Zas2011 
01037-7138 OGL 139     SMC114.7.13496 + SMC114.7.13580                                         Pli2012 
01037-7158 OGL 140     SMC113.5.9293  + SMC113.5.9288                                          Pli2012 
01038+2232 J   874     J measures a pair 1912 - 1917: 345@, 3".                                        
                       Measures and magnitude differences discordant.                          J__1949a
                       Companion has variable magnitude.                                       Cou1952a
01038+0122 STF  84     26 Cet.                                                                         
           STF  84     AB: H 4  83.                                                            MEv2010 
           BU 1355     AC: 1909 and 1921 measures disagree. BDS 494 same star.                         
01039-7255 SKF1068     OGL 141. SMC110.8.23710 + SMC110.8.23860                                Pli2012 
01040+3528 HO  213     A premature orbit has been calculated.                                          
01040-6409 B  1913     Spectrum composite: K0III/IV+A/F.                                               
01040-7134 OGL 142     SMC114.7.14379 + SMC114.6.11666                                         Pli2012 
01040-7401 OGL 143     SMC112.7.11    + SMC112.7.755                                           Pli2012 
01041+4408 UC  493     Not a CPM pair. The A component is a close double, leading to a                 
                       spurious proper motion (Skiff, private comm.).                                  
01042+2256 GIC  19     G069-044/G069-043.                                                              
                       NLTT 3529/3528                                                          Chm2004 
01044-0518 STF  85     Probably the same as STF 211 with a 1 hr error in RA.                           
01044-4703 UC  495     AB and BC are probably not CPM pairs. The proper motion of the B                
                       component was effected by a nearby bright star (Skiff, private comm.).          
01047+0401 GWP 126     XMI 168.                                                                Tob2012b
01047-3929 GJ 9037     Combined solution, based on reduction of Hipparcos intermediate                 
                       astrometric data together with spectroscopic elements from the Geneva           
                       Extrasolar Planet Search Programs home page.                            HaI2001 
01048+0135 A  2310     Position angles vary widely. A premature orbit has been calculated.             
01048-0528 STF  86     AB: H 3  73.                                                            MEv2010 
01049+3649 A  1515     Periods from 86 to 419yr have been calculated. Possibly ambiguous case          
01050+2119 LDS3228     NLTT 3570.  White dwarf pair = WD 0102+21 = EGGR 462/463                Grn1986 
01050-7132 OGL 144     SMC114.3.186   + SMC114.3.569                                           Pli2012 
01051+3814 J  1804     ALI 488.                                                                        
01051+1457 HJ 1068     72 Psc. A is a spectroscopic binary.                                            
01052+1250 HJ   10     Primary is eclipsing binary of Algol-type, period 1.62785 d.            Zas2012 
01053-7331 OGL 145     SMC111.8.20419 + SMC111.8.20441                                         Pli2012 
01055+8315 MLR 482     Also known as TDS  39.                                                          
01055+4928 ES 1206     1deg error in IDS led to similar error in WDS designation.                      
01055+1523 STF  87     NLTT 3597/3598                                                          Chm2004 
01055-7215 OGL 146     SMC113.2.30    + SMC113.2.126                                           Pli2012 
01056+4927 OSO  12     G172-038. Neither is a common proper motion pair, based on color and            
                       comparison with POSS2 red plates                                        Oso2004 
01056-7342 OGL 147     SMC112.5.12714 + SMC112.5.12879                                         Pli2012 
01057+2128 STF  88     psi 1 Psc                                                                       
                       AB: HJL  12.                                                            HJL1986 
                       AB: SHY 395. Bayesian analysis by Shaya & Olling (2011) indicates very  Shy2011 
                       high (near 100%) probability pair is physical.                                  
                       AB: H 4   9.                                                            MEv2010 
           YR    6     Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and                  
                       spectroscopic masses 4.29 +/- 0.78, 4.29, and 2.19 Msun, respectively.  Mlk2012 
01058+0455 STF  90     77 Psc. STTA 10. B is BD+04@176.                                                
                       AB: HJL  13.                                                            HJL1986 
                       AB: H 4  68.                                                            MEv2010 
01058-2618 HJ 2014     LDS  34. HIP 5140. See Allen et al. (2000) for information on           AlC2000 
                       metallicity, age, galactic orbital parameters, etc.                             
01058-5959 R     5     B is CPD-60@75.                                                                 
01058-7150 OGL 148     SMC114.1.170   + SMC114.1.1973                                          Pli2012 
01060+6120 LDS3230     Old LDS6109. Due probably to a typo in the epoch-1900 IDS coordinates,          
                       LDS3230 was originally listed in the WDS as 00055+6119.                         
01060+2456 BRT 122     J 2708.                                                                 J__1955 
01060+1111 BPM  21     [PM2000]   41785 + [PM2000]   41845.                                    Gvr2010 
01061-4643 SLR   1     bet Phe. Variable?                                                              
                       Quoted errors in P and a are +/- 5.0y and +/- 0.016", respectively.     Ary2015b
01062+3211 S   393     sig 2 Psc                                                                       
                       AB: H 5  16.                                                            MEv2010 
01065+5325 ES  616     One degree error in WDS designation - should be +5425.                          
01065+0154 HDO  42     Doolittle may have measured a different pair (see ADS).                 A__1932a
01065-3055 LDS2167     NLTT 3662/3663                                                          Chm2004 
01065-3441 LDS9110     Old LDS6110.                                                                    
01066+1353 SHY 396     HIP   5207 + HIP   4387.                                                        
01069-1408 GAL 306     Object #34 in Gallo's original list.                                    Gal1912a
01071+1740 BPM  22     [PM2000]   42380 + [PM2000]   42414.                                    Gvr2010 
01072+5330 H 4  66     H IV 66.                                                                        
01072+3839 A  1516     AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 2.62 +/- 0.59, 2.89, and 1.10 Msun, respectively.  Mlk2012 
01072-0144 STF  91     B is 2mag above the MS in (K,V-K), on MS in (J,J-K). Wrong 2MASS ptm.           
                       The B component is possibly a SB.                                       Tok2014d
01072-7121 OGL 149     SMC114.4.6097  + SMC114.4.6144                                          Pli2012 
01073+0537 GWP 130     XMI 169.                                                                Tob2012b
01073-7201 OGL 150     SMC113.3.21615 + SMC113.3.21614                                         Pli2012 
01074+0101 LDS5315     Error in WDS designation - incorrect precession of Luyten coordinates?  Luy1984 
01075+4116 RAO  40     Primary is SB, P=49.480d. Estim. mass of B 0.26 Msun.                   Tok2014d
                       Triple system with inner 74.1 day spectroscopic pair (Gorynya &                 
                       Tokovinin 2014 MNRAS 441, 2316) and tertiary from Riddle et al. (2015)  RAO2015 
                       confirmed as physical by our photometry and astrometry. Observations            
                       demonstrate that photometry of B given in 2MASS is biased by proximity          
                       of bright primary, as in many other similar pairs. Their "unusual"              
                       colors derived from the 2MASS photometry are thus wrong.                Rbr2015d
01075+0244 GWP 131     XMI 170.                                                                Tob2012b
01075-4145 LDS9111     Old LDS6111.                                                                    
01076+2257 LDS9112     AB: Old LDS6112.                                                                
                       NLTT 3723/3725                                                          Chm2004 
01078-4129 RST3352     ups Phe. Variable RV suspected. The lines are poor and show a scatter           
                       of 40km/s without apparent relation to the visual motion.                       
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 3.16 +/- 0.34, 2.78, and 2.09 Msun, respectively.             Mlk2012 
01079-7311 OGL 151     SMC111.3.12611 + SMC111.3.12798                                         Pli2012 
01080+3915 RAO  41     Primary is SB, P=1713d.                                                 Tok2014d
01083+5455 WCK   1     Aa,Ab: mu Cas = 30 Cas. Proper motion of A +3424 -1596 (FK5).                   
                       Aa,Ab: Malkov et al. (2012) derive dynamical, photometric, and                  
                       spectroscopic masses 0.01 +/- 0.01, 1.22, and 0.95 Msun, respectively.  Mlk2012 
           mu Cas      Aa,Ab: Astrometric orbit. Spectroscopic elements are somewhat                   
                       different from those of Lippincott: P = 23.0, T = 1954.0, e = 0.30,     Lip1981 
                       omega = 178.0 (Worek & Beardsley 1977).                                 Bey1977 
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       The pair has now been resolved by infrared speckle interferometry.      Mcy1983 
                       Pierce & Lavery (1985), Karovska et al. (1986), Haywood et al. (1992),  Pie1985 
                       and McCarthy et al. (1993) all compare their observations with          Kar1986b
                       published orbits and discuss  luminosities and masses of components,    Hay1992 
                       helium abundances, etc.                                                         
                       Hipparcos astrometric solution adopts some elements from the orbit      HIP1997d
                       of Heintz & Cantor (1994).                                              Hei1994b
           STT 551     AB: Optical pair, based on study of relative motion of the                      
                       components using the method of apparent motion parameters.              Kiy2008 
01083-3535 FAR   2     SKF 328. Primary is white dwarf WD 0106-358 = GD 683.                   Far2005b
01084+0539 BUP  15     80 Psc. B is BD+04@192.                                                         
           STT 552     AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
01084-5515 RST1205     zet Phe. A is an Algol-type system, spectrum composite, P = 1.67d.              
                       Both B and C are probably physical.                                             
                       Ling (2004) gives a derived orbital parallax 0".01176 and a mass sum    Lin2004a
                       of 7.41 +/- 5.85 Msun                                                           
01085+6331 OSO  13     G243-062. Not a common proper motion pair, based on comparison with             
                       POSS2 red plates. PM of A = +1047 -91.                                  Oso2004 
01086+1652 GWP 135     XMI 171.                                                                Tob2012b
01086+1917 GWP 136     XMI 172.                                                                Tob2012b
01086-1011 BUP  16     eta Cet = 31 Cet. B is BD-10@239.                                               
01088+6145 ES 1945     Aka OL  113.                                                                    
01088-7119 OGL 152     SMC119.5.5     + SMC119.6.162                                           Pli2012 
01089+4512 HJ 2018     AB,C : Same as STF  92.                                                         
01091-7225 OGL 153     SMC118.8.502   + SMC113.1.14118                                         Pli2012 
01092-7127 OGL 154     SMC119.6.1012  + SMC119.6.1006                                          Pli2012 
01093+6234 LDS5179     old LDS6113.                                                                    
01094+3543 BUP9005     A component is NGC 404.                                                 Skf2013 
01094+2949 ALP   4     2MASSW J0109216+294925                                                          
                       Physical companionship to this ultracool dwarf ruled out based on I-J           
                       color, using I-band photometry taken at WIYN in August 2002.            AlP2007 
01094+0457 GWP 138     XMI 173.                                                                Tob2012b
01094-5636 HU 1342     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.71 +/- 0.86, 2.48, and 1.27 Msun, respectively.             Mlk2012 
01095+4715 STT 515     phi And = 42 And. Measure of 1985.830 made by MAPPIT.                   Han1987 
                       Scardia et al. (2001) orbit considered preliminary.  The real period    Sca2001d
                       is probably long (>400 yr).  The Hipparcos parallax is 0".00443 +/-             
                       0.00080, giving a mass sum of 6.9 Msun, slightly in excess for a                
                       binary of spectral type B7Ve. The dynamical parallax is 0".0033, in             
                       reasonable agreement with the measured one but not acceptable as it             
                       leads to an exaggerated mass sum (16.8 Msun).                                   
                       Calculated mass sum is 6.5  +/- 2.8 Msun, in reasonable agreement with          
                       spectral types B6IV and B9V, although mass is not well-constrained.     Mut2010b
01096+4635 ES 1300     Due to a typographical error in the ADS, the AE, AF, AG, AH, and AI     A__1932a
                       components of 01097+3537 were added as additional components to this            
                       pair (the AE and AI pairs as BAR  66, the others as ES 1300).                   
01096+2802 BRT 123     OL  149.                                                                        
01096-0507 LDS9114     Old LDS6114. LIT   3.                                                           
                       NLTT 3847/3849                                                          Chm2004 
01096-0711 HDS 151     This binary displays clear common proper motion, but the residual               
                       astrometry does not seem to follow a simple trajectory consistent with          
                       only orbital motion of the two visible components. In addition, the             
                       brightness difference is larger than the spectral type difference               
                       would imply at a common distance. This could indicate that the A                
                       component is itself an unresolved binary.                               Jnn2012 
01097+3537 BAR   1     bet And = 43 And = Mirach                                                       
                       Also, see note to 01096+4635.                                                   
01097+0856 GWP 139     XMI 174.                                                                Tob2012b
01098-2013 HJ 2023     Primary is CT Cet, a W UMa type eclipsing binary, P = 0.25649d.         Zas2012 
01099+1352 BPM  23     [PM2000]   44058 + [PM2000]   44035.                                    Gvr2010 
01100-7327 OGL 155     SMC111.2.5925  + SMC111.2.6033                                          Pli2012 
01101+5145 STT  23     AB: HJL  14.                                                            HJL1986 
01102+2447 POU 107     J 1805.                                                                         
01104-7352 OGL 156     SMC112.3.6394  + SMC117.6.1318                                          Pli2012 
01105+1326 BPM  24     [PM2000]   44379 + [PM2000]   44460.                                    Gvr2010 
01105+1019 GWP 143     XMI 175.                                                                Tob2012b
01107+8021 STF  89     B is BD+79@32.                                                                  
01107-2800 SWR   1     CPM pair                                                                Skf2004 
01108+6747 HDS 155     A spectroscopic double lined orbit has been determined as well.         Grf2012d
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.02 +/- 0.23, 2.18, and 2.52 Msun, respectively.             Mlk2012 
01108+5141 DOO   3     BDS 631.                                                                        
01109+0934 HJ  634     Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01111+5509 STT 553     the Cas = 33 Cas. A is a spectroscopic binary,                                  
                       Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01111+3125 STT  25     82 Psc = g Psc                                                                  
01111-7228 SKF1069     OGL 157. SMC115.5.12    + SMC115.5.319                                  Pli2012 
01112+4113 A   655     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.59 +/- 0.83, 2.76, and 0.95 Msun, respectively.             Mlk2012 
01112+3743 HO  215     45 And. Also single 1903, 1906 (Doolittle), 1907 (Aitken).                      
                       A measure by Schembor (1925.60, 117.8@, 155.5", 6 - 6) belonged to      Sch1927a
                       01107+4256 ENG   4AB instead.                                                   
                       Duplicity of A is questionable.                                                 
01112+1634 GWP 144     XMI 176.                                                                Tob2012b
01114+1526 BEU   2     GJ 3076. WDS designation incorrected entered as 01224+1526.                     
                       Estimated age 10-20 Myr; masses 0.10 +/- 0.03 and 0.04 +/- 0.01 Msun;           
                       a ~5.6 au.                                                              Jnn2014 
01114-7225 OGL 158     SMC118.8.10104 + SMC118.8.10016                                         Pli2012 
01114-7323 OGL 159     SMC116.7.144   + SMC116.7.143                                           Pli2012 
01116+0446 GWP 146     XMI 178.                                                                Tob2012b
01116+1404 GWP 145     XMI 177.                                                                Tob2012b
01117+1205 LDS3242     NLTT 3967/3952                                                          Chm2004 
01119+0455 GIC  20     G002-027/G070-044 = GJ 3077A+3078B.                                             
01120+0642 GWP 149     XMI 180.                                                                Tob2012b
01120+0955 GWP 148     XMI 179.                                                                Tob2012b
01120-7231 OGL 160     SMC115.5.9132  + SMC115.5.9369                                          Pli2012 
01121+6111 KR   10     AC: Doolittle's published position angle was 91.9deg, which does not    Doo1901 
                       match anything in the field. However, an obvious star is visible at             
                       the same separation but 90deg off his theta measure. It is assumed he           
                       made an error when rotating his micrometer.                                     
           SMA9001     AD: Doolittle noted "a 13.5 mag. companion about 7" from A was          Doo1901 
                       suspected on two nights". It is assumed he saw the Smart companion.     Sma1932 
01121+4700 BU  236     Aka HJ 2024.                                                                    
01121-7400 OGL 161     SMC117.7.58    + SMC117.3.98                                            Pli2012 
01125+0228 STT  27     35 Cet                                                                          
01126+1704 NAU   1     The primary is GU Psc, a likely member of the young AB Doradus Moving           
                       Group. Spectral types are M3 +/- 0.5 and T3.5 +/- 1. Age of the system          
                       is 100 +/- 30 Myr, distance 48 +/- 5 pc.                                Nau2014 
01129+3205 STF  98     B is BD+31@196a. The primary is a double-lined spectroscopic binary,            
                       P = 2.21d. B may also be an SB (Hube, PASP 93, 490; 1981).                      
                       AB: H 4 120.                                                            MEv2010 
                       SEI  13.                                                                Nsn2017a
01130+3004 STT  26     A is a spectroscopic binary.                                                    
01131+2942 A  1260     Angle increasing, with a probable close approach about 1950.                    
01131+1141 HD  7275    Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
01131-7215 OGL 162     SMC118.2.51    + SMC118.2.127                                           Pli2012 
01132-7400 OGL 163     SMC117.7.3315  + SMC117.7.3338                                          Pli2012 
01133-0152 HIP   5697  The SB1 orbit suggests mass ratio q > 0.2 and axis 0".21. The companion         
                       is probably just a bit too faint or too close to be resolved with NICI. Tok2012a
01134-3932 SHY 397     HIP   5709 + HIP   5490.                                                        
01134-7251 OGL 164     SMC115.2.45    + SMC115.2.260                                           Pli2012 
01135-3821 BRG   4     The primary star in the system is a known eclipsing binary with a               
                       period of 0.4455 days (Parihar et al. 2009 MNRAS 395, 593). Since the           
                       angular separation is inside of our inner cut-off, we count the system          
                       as a binary here for the purpose of multiplicity statistics, although           
                       it is really a triple system. To estimate the mass of the primary for           
                       the purpose of deriving the mass ratio to the tertiary component                
                       detected in our images, we use the sum of the masses corresponding to           
                       individual spectral types M1 and M3 derived for the eclipsing binary.   Jnn2012 
                       ASAS J011328-3821.1, eclipsing binary of Algol type, period 0.44559d.   Zas2016 
01136+2825 HJ  635     Previously erroneously listed as 01126+2825.  Also known as GRV  73.            
01137+2435 STF  99     phi Psc = 85 Psc. A is a spectroscopic binary.                                  
01137+0735 STF 100     zet Psc. Both A and B are spectroscopic and occultation binaries, B             
                       has P = 9.08d.                                                                  
                       AB: HJL  15.                                                            HJL1986 
                       AB: H 4   8.                                                            MEv2010 
           BU 1029     BC: Delta m given in ADS is greatly overestimated.                      Wor1967b
01137-5040 HJ 3421     B is CD-51@312.                                                                 
                       Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01139+1004 GWP 154     XMI 181.                                                                Tob2012b
01141+1698 87 Psc      Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Stickland & Weatherby (1984).                                           Stc1984 
01141+0634 LDS3248     LDS5323.                                                                        
01142-4041 B  2554     Hipparcos suspected non-single.                                                 
01144-0755 STFA  3     37 Cet = LDS3250. B is BD-08@215.                                               
                       NLTT 4123/4121                                                          Chm2004 
                       AB: GJ 9045 A+B. CPM pair.                                              Mkr2008 
                       AB: H 5  24.                                                            MEv2010 
01144-7319 OGL 165     SMC116.3.3     + SMC116.3.954   + SMC116.6.11112                        Pli2012 
01145-0503 ROL   1     Primary is exoplanet host, periods 1275d, 4046d.                        Tok2014d
           RGS   1     Aa,Ab: HD 7449 has a close massive planet (P = 1270.5 +5.92/-12.1d,             
                       a =  2.33 +0.01/-0.02 au, mass >1.09 +0.52/-0.19 Mjup) as well as a             
                       more distant stellar companion. The Ab component is likely an M4-M5             
                       dwarf. Rodigas et al. (2016) estimate P = 65.7 +227/-56y, a =  17.9             
                       +32/-12.9 au, i = 59.7 +20.1/-25.8 deg, mass = 0.23 +0.22/-0.05 Msun.   Rgs2016 
01146-7402 OGL 166     SMC117.7.3320  + SMC117.7.3907                                          Pli2012 
01148+6056 BU 1100     The quadrant interpretation by Zulevic is less likely.                  Zul1972a
                       Muller corrected an error in his elements (Ephem. Cat. 1964).           Mlr1955b
                       One component is a SB, P = 5.33d.                                               
                       Only elements P, T, and a have been amended by Starikova (1977) from    Sta1977a
                       the orbit of Zulevic (1972).                                            Zul1972a
01148+4309 LDS3251     NLTT 4129/4124                                                          Chm2004 
01148-0058 BUP  18     38 Cet.                                                                         
                       A is a blue supergiant with multiple pulsation periods.                 IAU2014e
                       AC: C component is galaxy NGC 442.                                              
01149+3236 SEI  14     None of the components seen on POSS plate; may be flaws on AC Potsdam           
                       plate. The current WDS companion at the position of Scheiner's triple           
                       is probably unrelated to anything seen on the plates.                           
                       AC: SEI  15.                                                            Nsn2017a
01152-3419 LDS 837     LDS5325.                                                                        
01153+6040 LDS5180     old LDS6115.                                                                    
01153+2234 J  3226     BRT2304. Barton lists theta as 226.9; probably typo for 266.9.          Brt1939b
01155+3745 SHY 121     HIP   5881 + HIP   6278.                                                        
                       A: Ren & Fu (2013) calculated an astrometric orbit, combining                   
                       Hipparcos Intermediate Astrometric Data with spectroscopic elements by          
                       Nidever et al. (2002). They derived component masses 0.95 and 0.28      Nid2002 
                       Msun and an estimated semimajor axis of 30.68 mas.                      Ren2013 
01155+0216 CHR 195     First detected as an occultation binary by Evn1983a.                            
01157+0241 GWP 157     XMI 182.                                                                Tob2012b
01157+0032 LDS5326     Error in WDS designation - incorrect precession of Luyten coordinates?  Luy1984 
01158+4702 LAW   9     LSPM J0115+4702S. Law et al (2008) derive a distance of 18.7 +9.3/-3.6  Law2008 
                       pc and a projected separation of 5.2 +2.9/-0.9 au. Estimated spectral           
                       types are M4.5 and M5.                                                          
                       In addition to the companion detected with AstraLux, it can be noted            
                       that 2MASS J01154885+4702259 has a very similar proper motion to the            
                       star J01155017+4702023 at just 27" separation (Roser et al. 2010),      Rsr2010 
                       which is itself a close binary (Law et al. 2008). Thus, this is a very  Law2008 
                       likely quadruple system.                                                Jnn2012 
01158+0947 A  2102     Quadrant change. Not seen 1948 - 1954.                                          
01158-6853 HJ 3423     kap Tuc = LDS  42.                                                              
           I    27     HJ 3423 and I 27, separated by 320", form the quadruple system                  
                       kap Tuc. The position of I 27 is 011501.0-684908 (2000).                Sca1981a
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
01158-7224 OGL 167     SMC118.1.5565  + SMC118.1.6020                                          Pli2012 
01160+5849 STI1550BC   Aka MRI  29.                                                                    
01160+1534 GRV 986     SLW  58.                                                                        
01162-7246 OGL 168     SMC115.2.6083  + SMC115.2.6082                                          Pli2012 
01163+1243 BPM  25     [PM2000]   47807 + [PM2000]   47744.                                    Gvr2010 
01163-2056 LDS  41     NLTT 4238/4239                                                          Chm2004 
01163-3217 LDS1091     LDS5327.                                                                        
01166+7402 HJ 2028     STTA 13.                                                                        
01166+1831 HDS 169     A: Ren & Fu (2013) calculated an astrometric orbit, combining                   
                       Hipparcos Intermediate Astrometric Data with spectroscopic elements by          
                       Latham et al. (2002). They derived component masses 1.06 and 0.28 Msun  Lat2002 
                       and an estimated semimajor axis of 14.81 mas.                           Ren2013 
01166+1507 GWP 161     XMI 183.                                                                Tob2012b
01166-0230 BU 1358     39 Cet. A semiregular variable, AY Cet, and spectroscopic binary, P =           
                       56.8d. Radio flares and soft X-rays are observed, and a white-dwarf             
                       companion is revealed by IUE observations.                                      
01167-7142 OGL 169     SMC124.7.387   + SMC124.7.163                                           Pli2012 
01168+2643 BRT3257     Originally published as BRT 124.                                        Brt1928 
01170-7311 OGL 170     SMC116.3.7036  + SMC116.3.7122                                          Pli2012 
01171+1739 BPM  26     [PM2000]   48328 + [PM2000]   48320.                                    Gvr2010 
01171-7355 OGL 171     SMC117.3.682   + SMC117.3.1102                                          Pli2012 
01172+0930 GWP 164     XMI 184.                                                                Tob2012b
01175+0131 GWP 165     XMI 185.                                                                Tob2012b
01176+4018 A  1521     Rapid change, but the measures are inadequate to define the motion.             
01177+2647 BRT3258     Originally published as BRT 125.                                        Brt1928 
01177-7150 OGL 172     SMC124.8.4147  + SMC124.8.4560  + SMC124.8.4191                         Pli2012 
01178+4945 HU  520     Quadrant indeterminate.                                                         
01178+4901 HJ 2033     Ea : Also known as STF 102 ET.                                                  
01179-7314 OGL 173     SMC116.3.7181  + SMC116.3.7479                                          Pli2012 
01180+0037 GWP 167     XMI 186.                                                                Tob2012b
01181+4707 A   937     North preceding and slightly brighter of a finder pair. Narrow                  
                       apparent orbit.                                                         B__1963b
01182+1409 BPM  27     [PM2000]   48977 + [PM2000]   49004.                                    Gvr2010 
01182-7136 OGL 174     SMC124.7.4469  + SMC124.7.4898                                          Pli2012 
01184-2332 LDS2182     Appears to be same as SKF1373. Primary is B component of 01183-2330             
                       SKF1372; pair moved to become AC pair (with quadrant flip).                     
01185+7323 A   814     Not separated about 1951 (Van Biesbroeck). Possible quadrant change.    VBs9999 
01186+3855 GIC  21     G132-069/G132-068.                                                              
                       NLTT 4342/4337                                                          Chm2004 
01186-2255 FAR  24     Primary is white dwarf WD 0116-231.                                     Far2006 
01187-0052 HJ 5453     LDS  43. HIP 6130. See Allen et al. (2000) for information on           AlC2000 
                       metallicity, age, galactic orbital parameters, etc.                             
                       AB: NLTT 4362/4361                                                      Chm2004 
           EGN   1     Aa,Ab pair bound. Colors of Ab component consistent with M2-M5 dwarf,           
                       with mass 0.24 +/- 0.01 Msun.  B component is K7 dwarf and shares               
                       CPM with A. C component is likely a background star.                    Egn2007 
01187-2249 HDO  47     Probably = HDO 48.                                                              
01188+3724 STF 108     The A component is a spectroscopic binary.                                      
01188-5637 RST  29     Spectral type G5?                                                               
01191-7215 OGL 175     SMC123.7.2850  + SMC123.7.2849                                          Pli2012 
01192+5821 STI1560     B is BD+57@248.                                                         FMR9999 
01192-4338 B  1423     Zurlo et al. (2013) estimate the period of this system at ~300y, in an          
                       eccentric orbit with a semi-major axis of ~50au. The companion is               
                       likely a white dwarf.                                                   Zur2013 
01194+6418 MLB 186     TDS1841.                                                                        
01194+1158 BPM  28     [PM2000]   49715 + [PM2000]   49656.                                    Gvr2010 
01194-7129 OGL 176     SMC124.3.274   + SMC124.3.22                                            Pli2012 
01194-7246 OGL 177     SMC120.7.5025  + SMC120.8.5604                                          Pli2012 
01194-7359 OGL 178     SMC122.7.221   + SMC122.7.232                                           Pli2012 
01195+5816 ES  408     CD component also known as STI1562                                              
01195+1850 GWP 169     XMI 187.                                                                Tob2012b
01195-7205 OGL 179     SMC123.6.2701  + SMC123.6.3359                                          Pli2012 
01196-0520 A   313     Only elements P and T have been amended by Starikova (1977) from the    Sta1977a
                       orbit of Heintz (1968).                                                 Hei1968a
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.39 +/- 1.07, 2.59, and 1.10 Msun, respectively.             Mlk2012 
01197+1209 CHR 196     First detected as an occultation binary by Africano.                    Afr1975 
01197-7203 OGL 180     SMC123.6.2671  + SMC123.6.3140                                          Pli2012 
01198-0031 STF 113     42 Cet.                                                                         
                       AB: Absolute quadrant for 1998.657 determined by triple-correlation             
                       techniques.                                                             Pru2002b
                       A,BC. 1985.8430: This autocorrelogram was remeasured; the new results           
                       are listed in catalog.                                                          
                       Star A (mag. 6.3, G8III) is in slow direct motion at 1.6" separation.           
                       T incorrectly given as 1992.52 by Baize (1990); should be 1993.02       Baz1990a
                       (erratum noted in Inf. Circ. 111, 1990)                                         
           FIN 337     BC: 1982.7629, 1982.7657, 1983.7106: A mistake in reduction resulted in         
                       90 degree errors for these three measures.                              McA1987b
                       BC: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 1.79 +/- 0.56, 3.32, and 1.20 Msun, respectively.  Mlk2012 
01198-7157 OGL 181     SMC123.5.2462  + SMC123.5.2499                                          Pli2012 
01199+0350 CHE  29     BAL2084.                                                                Hln1972 
01200+5747 STI1571     Aka LYS   5. Identity not recognized due to large pm affecting pa.              
01200-1549 HJ 2036     A is an SB. Binary or triple?                                           Tok2014d
01201+5814 H 3  23     H III 23. phi Cas = 34 Cas. A is a spectroscopic binary.                        
                       A quintuple system. C has spectral type B5/6Ia/be.                              
01201+3900 GIC  22     G132-071/G132-072.                                                              
                       NLTT 4410/4412                                                          Chm2004 
01203-0933 LDS9116     Old LDS6116.                                                                    
01203-4841 HJ 3428     B is CD-49@378.                                                                 
01204+0937 GWP 171     XMI 188. BVD  15.                                                       Tob2012b
01205+0418 J  1807     BAL 2085.                                                                       
01205-1957 TOK 203     Two astrometric orbits are derived by Goldin & Makarov (2006), the      Gln2006 
                       longest one has P = 8.93 yr, axis 55 mas, and e = 0.84.                 Tok2012a
                       Retrograde motion by 4deg since first resolution in 2011. Goldin &              
                       Makarov (2006) propose two orbits with periods ~9yr; semi-major axis    Gln2006 
                       should then be 0".15, so the system is near apastron.                   Tok2013b
01207+0333 GWP 172     XMI 189.                                                                Tob2012b
01207-7145 OGL 182     SMC124.1.101   + SMC124.1.545                                           Pli2012 
01208+1127 AG   17     LDS 878. B is BD+10@167.                                                        
                       HJL  17.                                                                HJL1986 
01208+1035 PLQ  13     B is BD+09@153.                                                                 
                       HJL  16.                                                                HJL1986 
01211+6439 S   397     35 Cas. STTA 15 = H 5  81.  B is BD+63@175.                                     
                       Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01211+1540 J   227     B is variable                                                           Cou1952a
01211+0736 SLE 257     The primary is a W UMa system, AQ Psc.                                          
01211-0403 LDS3267     G 271-42.                                                                       
01211-3508 LDS5330     Aka LDS9117 the old LDS6117.                                                    
01211-7251 OGL 183     SMC120.2.15    + SMC120.2.163                                           Pli2012 
01211-7305 OGL 184     SMC121.5.2620  + SMC121.5.3200                                          Pli2012 
01212+5159 NLTT 4450   Ren & Fu (2013) calculated an astrometric orbit, combining Hipparcos            
                       Intermediate Astrometric Data with spectroscopic elements by Latham et          
                       al. (2002). They derived component masses 1.21 and 0.26 Msun and an     Lat2002 
                       estimated semimajor axis of 35.17 mas.                                  Ren2013 
01212+4108 LDS3266     NLTT 4468/4469                                                          Chm2004 
01213+1132 BU    4     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       The Hipparcos parallax (0".00616 +/- 0.00141) yields a mass sum of      Sca2001d
                       4.7 Msun, in excess for a binary of type F1III.                                 
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 9.73 +/- 6.50, 3.62, and 1.64 Msun, respectively.  Mlk2012 
01215-2908 RUC   1     BE Scl. Spectral type of resolved companion estimated at G5-8V.         Ruc2007 
01218-2408 SEE  13     Motion direct. A premature orbit has been computed.                             
01219-4003 WG    8     BRT 643.                                                                Brt1933 
01220+1848 GWP 175     XMI 190.                                                                Tob2012b
01220-6943 I   263     A premature orbit has been computed. Motion direct.                             
01221-2654 LDS2189     NLTT 4564/4566                                                          Chm2004 
01223+0331 DEA  38     NLTT 4558 + 2MASS J01221697+0331235. Baron et al. (2015) estimate               
                       spectral types G5 and L2 +/- 1, distances 58 +/-3 and 43 +13/-40 pc,            
                       masses 1.05 -1.12 and 0.071-0.076 Msun.                                 BFr2015 
01223-7332 OGL 185     SMC121.1.5     + SMC121.1.187                                           Pli2012 
01226+1200 GWP 178     XMI 191.                                                                Tob2012b
01227+1410 GWP 179     XMI 192.                                                                Tob2012b
01227+0032 LDS3270     Aka WNO  42.  G 70-55.                                                          
01227-7258 OGL 186     SMC120.1.13    + SMC120.1.32                                            Pli2012 
01228-2440 BWL  63     Bowler et al (2013) derive the following properties: age 120+/-10 Myr,          
                       distance 36+/-4 pc, masses 0.40+/-0.05 Msun and 12-14 or 23-27 Mjup.    Bwl2013 
01230-1258 GAL 307     LDS  46. Object #40 in Gallo's original list.                           Gal1912a
           KUI   6     BC: BC shares CPM with A.                                               B__1963b
01230-3035 LDS2190     According to Richard Jaworski the precise position he determine may be  Jaw2006 
                       correct if Luyten's original separation is off by an order of                   
                       magnitude (i.e., 11.8" rather than 118").                                       
01232+4905 KU    8     HU 524.                                                                         
01233+0152 LDS5332     CVR  26.                                                                        
01233-0209 LDS3271     NLTT 4616/4615                                                          Chm2004 
01233-2105 LDS2191     NLTT 4626/4625                                                          Chm2004 
01233-7256 OGL 187     SMC120.1.3850  + SMC120.1.4139                                          Pli2012 
01234+5809 STF 115     First measured by F.W. Struve in 1836 at an angular separation of       Hrt1989 
                       0".68, this system had opened to 1".2 by 1910, then steadily closed             
                       to 0".35 at the time of the first speckle measurement in 1978.                  
                       The pair reached an apparent minimum separation of 0".01 in the                 
                       spring of 1984.                                                                 
                       1983.7107  This autocorrelogram was remeasured; the new results are             
                       listed in the catalog.                                                          
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 2.36 +/- 0.67, 2.80, and 1.20 Msun, respectively.  Mlk2012 
01235-7356 OGL 188     SMC122.3.2     + SMC122.3.173   + SMC122.5.71                           Pli2012 
01236+3415 CRJ   4     NLTT 4619. The A component is SB, P=83.9d. Primary is G8IV. The 0.3"            
                       companion is physically associated with primary, based on multi-epoch           
                       astrometry. The estimated spectral type of the companion ~M1V, its              
                       mass > 0.297 Msun.                                                      CrJ2013 
01236+0753 GWP 180     XMI 193.                                                                Tob2012b
01237-6217 RST  31     Spectral type G0?                                                               
01239+0050 GWP 182     XMI 194.                                                                Tob2012b
01239-7228 OGL 189     SMC120.4.3345  + SMC120.4.3627                                          Pli2012 
01240-0800 HJ 1079     44 Cet. A is a Delta Scuti-type variable, AV Cet.                               
01240-0811 BU  505     the Cet = 45 Cet.                                                               
01240-2933 LDS2192     NLTT 4676/4656                                                          Chm2004 
01241-1244 GAL 308     Object #42 in Gallo's original list.                                    Gal1912a
01242+1254 HJ   13     C component is galaxy NGC 514.                                                  
01243+0426 GWP 183     XMI 195.                                                                Tob2012b
01243-0655 BU 1163     The system is also detected as a spectroscopic binary.                  B__1951a
                       Only elements P, T, and a have been amended by Starikova (1978) from    Sta1978c
                       the orbit of van den Bos (1961).                                        B__1961e
                       This system underwent periastron in late 1988, an event now covered by          
                       speckle observations.                                                   Hrt1992b
                       A combined visual-spectroscopic orbit by Morbey (1975) gives almost     Mrb1975 
                       the same elements, but in the representation of position angles         Sod1999 
                       Soderhjelm's elements are preferable.                                           
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.59 +/- 0.41, 2.74, and 1.30 Msun, respectively.             Mlk2012 
01245+3902 STTA 17     B is BD+38@256.                                                                 
                       D is BD+38@253.                                                                 
01245+1740 BPM  29     [PM2000]   52622 + [PM2000]   52637.                                    Gvr2010 
01245-2839 LDS2194     NLTT 4694/4695                                                          Chm2004 
01245-3356 JAO   1     Aa,Ab: GJ 2022 = G274-024                                                       
                       Daemgen et al. derive a distance of 12.6 +/- 2.3 pc, a separation for           
                       the AC pair of 26.0 +/- 4.8 au, and a predicted orbital period of 330           
                       +95/-93 yr. Spectral types for both components are M5.0 +/- 0.5;                
                       masses are 0.14 +0.03/-0.02 and 0.13 +0.03/-0.02 Msun.                  Dae2007 
01246+5311 ES 2583     B is BD+52@332.                                                                 
01247-7402 OGL 190     SMC122.2.45    + SMC122.2.104                                           Pli2012 
01248-2614 RST1218     LDS 3277.                                                                       
                       NLTT 4714/4713                                                          Chm2004 
01250+1424 GWP 185     XMI 196.                                                                Tob2012b
01251+4537 A   939     Recent observations seem to rule out Muller's short-period              Mlr1955a
                       alternative.                                                                    
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.54 +/- 1.99, 3.23, and 1.45 Msun, respectively.             Mlk2012 
01252-0412 HJ  638     01252-0409BU 1361                                                               
                       J  1445.                                                                Nsn2016 
01252-7954 HJ 3443     B is CPD-80@23.                                                                 
01253-5930 HJ 3435     B is CPD-60@111.                                                                
01254+0227 GWP 186     XMI 197.                                                                Tob2012b
01256+3133 STT  30     AC: HJL  18. Aka MAD   9.                                               HJL1986 
                       AC: SHY 402. Bayesian analysis by Shaya & Olling (2011) indicates very  Shy2011 
                       high (near 100%) probability pair is physical.                                  
                       STTA 18.                                                                        
                       B is above MS (wrong ptm), while A and C are on it. C is SB2,           HJL2012b
                       P=14.908d (Halbwachs et al. 2012)                                       Tok2014d
01256+2331 TOK  11     Primary is 5.4d SB1. Estimated period of visual pair 880y.              Tok2006 
01257+0258 J  1899     BC: Error in coordinates listed in Jonckheere (1941), star is at        J__1941a
                       1h 23.2m, not 0h 23.2m.  Star of mag 7.3 at 131" is BD+02  207.         J__1952 
01257+0107 GWP 188     XMI 199.                                                                Tob2012b
01257+0611 GWP 187     XMI 198.                                                                Tob2012b
01258+6014 BUP  19     del Cas = 37 Cas = Ruchbah. A spectroscopic and (perhaps) eclipsing             
                       binary.                                                                         
01259+6808 BU 1101     psi Cas = 36 Cas.                                                               
           H 5  83     H V 83, SHJ 18, STF 117. C is BD+67@124.                                        
                       AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
01260+1450 BPM  30     [PM2000]   53515 + [PM2000]   53480.                                    Gvr2010 
01261+0925 GWP 189     XMI 200.                                                                Tob2012b
01261-2618 SWR   2     CPM pair                                                                Skf2004 
01262+3435 WSI  96     Provisionally designated WSI9101.                                       Tok2010 
                       The initial observations of WSI 96 by Mason et al. (2011) are           Msn2011d
                       considered spurous. The pair resolved by Roberts et al. (2015) using            
                       AO is believed to be a different pair, whose magnitude difference               
                       would have been beyond the dm limit of speckle. The original WSI 96             
                       designation was retained, however. Spectral types of the components             
                       are estimated as F7V and M2V, masses as 1.4 and 0.4 Msun.               Rbr2015b
01263+0711 LDS9118     Old LDS6118.                                                                    
01263-0440 TOK 204     Possible physical companion at 24".4, 227deg in 2MASS.                  Tok2012a
                       Direct motion by 20deg since first resolution in 2011, at constant              
                       separation. Estimated period ~10yr. The small RV amplitude suggests an          
                       orbit in the plane of the sky.                                          Tok2013b
01264+5929 STI 213     STI1607.                                                                        
01265+1812 HDS 187     Also a spectroscopic binary with P = 3087d which cannot be the visual   Grf2015b
                       pair.                                                                           
01267-7408 OGL 191     SMC122.1.1145  + SMC122.1.1144                                          Pli2012 
01269-5023 ART   1     Low-mass wide double, discovered on 2MASS and Digital Sky Survey                
                       frames. Artigau et al. determine sectral types M6.5V +/- 0.5 and M8V    Art2007 
                       +/- 0.5, distances 63 +/- 5 and 61 +/- 6 pc. Based on evolutionary              
                       models, the masses are 0.095 +/- 0.005 and 0.092 +/- 0.005 Msun for an          
                       age > 1Gyr, or 0.020 +/- 0.003 and 0.019 +/- 0.003 Msun for and age             
                       ~30Myr. The projected separation is ~5100 au.                                   
01270+1500 GWP 190     XMI 201.                                                                Tob2012b
01270+1200 LDS3282     G002-038. See Allen et al. (2000) for information on metallicity,       AlC2000 
                       age, galactic orbital parameters, etc. Also known as LIT   5.                   
                       NLTT 4817/4814                                                          Chm2004 
01270-0009 STF 125     Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01270-3058 RSS   3     This previously uncataloged double star was a Hipparcos double entry            
                       system.  The first measure is determined from the individual positions          
                       listed by Rousseau et al.                                               Rss1996 
                       SHY 403. Bayesian analysis by Shaya & Olling (2011) indicates very      Shy2011 
                       high (near 100%) probability pair is physical.                                  
01270-3233 LDS2199     Some unconfirmed early observations. A is the semiregular variable              
                       R Scl.                                                                          
01270-7405 OGL 192     SMC122.2.1199  + SMC122.2.1250                                          Pli2012 
01271-5158 SHY 404     HIP   6772 + HIP   6804.                                                        
01274-0204 J  1446     BAL 6.                                                                          
01274-2220 RST2261     CD-22@503.                                                                      
01275+1546 BPM  31     [PM2000]   54366 + [PM2000]   54359.                                    Gvr2010 
01276+6429 TDS1882     CD: Originally 01276+6430 TDS1882; primary found to be C component of           
                       01276+6429.                                                                     
01276+0402 GWP 192     XMI 202.                                                                Tob2012b
01277+6321 STI 215     MLB 382.                                                                        
01277+4524 BU  999     ome And = 48 And                                                                
                       This cannot be the close 254.9-d spectroscopic binary.                  Grf2011b
                       Although the pair has been repeatedly resolved with the CHARA Array             
                       with the Separated Fringe Packet technique, a full solution is not      CIA2010 
                       yet complete.                                                                   
           CIA   4     Aa,Ab: Combined solution by Farrington et al. (2014) yields masses              
                       0.993 +/- 0.056 and 0.888 +/- 0.058 Msun, as well as an orbital                 
                       parallax 39.12 +/- 1.97 mas (compared with the Hipparcos parallax of            
                       34.94 +/- 3.1 mas).                                                     CIA2014a
           BU   82     CD: There is a faint star between the AB and CD pairs. The change in            
                       AC is due to the proper motion of A. This is common to AB.              Bu_1894 
01277+1620 BPM  32     [PM2000]   54497 + [PM2000]   54549.                                    Gvr2010 
01277+0521 BU 1164     See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 2.51 +/- 0.76, 2.67, and 1.05 Msun, respectively.  Mlk2012 
01278+5928 STI1618     STI 217.                                                                        
01281-5238 CVN   2     Both the B and C companions are probably background objects.            Cvn2005a
01282+1244 GWP 193     XMI 203.                                                                Tob2012b
01283+5329 STF 123     AB: Also known as HU 1651, but the 1911 Hussey measure has a quadrant           
                       flip and a large sep error.                                             Hu_1911 
01283+1731 GWP 194     XMI 204.                                                                Tob2012b
01283+1429 AG   18     B is BD+13@217.                                                                 
01283-1615 LDS3284     NLTT 4889/4888                                                          Chm2004 
01284+0758 S   398     STTA 19. B is BD+07@214.                                                        
                       HJL  19.                                                                HJL1986 
01284-4319 gam Phe     Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Luyten (1936).                                                          Luy1936 
01287-4710 LDS  48     Aka UC  562.                                                                    
01289+0633 PLQ  16     LDS3285.                                                                        
01290+7412 HJ 2045     LDS1529.                                                                        
                       A is above MS, B on the MS. A component possibly a close double         Mkr2005 
                       (Makarov & Kaplan 2005) but nothing on the close sub-system in SIMBAD.  Tok2014d
01291+2143 HO    9     BC: According to Griffin, the radial velocities of B and C differ by    Grf1987c
                       30km/sec. Either the pair is optical, or one component is a                     
                       spectroscopic binary.                                                           
                       AB and AD: Optical pairs, based on study of relative motion of the              
                       components using the method of apparent motion parameters.              Kiy2008 
01291+1040 GWP 195     XMI 205.                                                                Tob2012b
01292+4820 BWL   6     AC: Source appears spatially extended; probably a background galaxy.            
                       Primary is G 172-56.                                                    Bwl2015 
01295+6319 MLB 330     This pair was purged from an earlier edition of the WDS as it was not           
                       found by Heintz. It has apparently been located. It and the nearby              
                       MLB 329 are in NGC 559.                                                 Hei1985a
01295+3054 BUP  20     B is BD+30@229.                                                                 
01296-2138 SEE  14     48 Cet.                                                                         
01297+4228 ZUC   6     SKF 314.                                                                        
                       Primary is white dwarf WD 0126+422 = GD 13.                             Zuc1992 
01297+2250 A  1910     AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 6.11 +/- 1.86, 4.31, and 2.09 Msun, respectively.  Mlk2012 
01298+1014 CHR 197     First detected as an occultation binary by Africano.                    Afr1977b
01299+3100 ENG   6     B is BD+30@232.                                                                 
01300-2231 I   445     A,BC = LDS  51.                                                                 
01302+0609 STH   6     A: mu Psc = 98 Psc                                                              
01305-4242 I  1609     SY Phe, an Algol type eclipsing binary, P = 5.27095d.                   Zas2012 
01306-4446 DHI   1     At a distance of 40 +/- 14pc, the projected physical separation is 130          
                       +/- 50au. Spectral types are M9.0 +/- 0.5 and L6 +/- 1. Dhital et al.           
                       conclude the pair is physical.                                          Dhi2011 
01307-1227 GAL 309     Object #45 in Gallo's original list.                                    Gal1912a
01309+5244 GIC  23     G173-002/G173-003.                                                              
                       NLTT 4991/4993                                                          Chm2004 
01312+7016 38 Cas      Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Wright & Pugh (1954).                                                   Wri1954 
01315+1521 BU  506     eta Psc = 99 Psc. A is a Beta CMi-type variable.                        Baz1964 
01316-1901 HJ 2052     B is BD-19@263. BDS 796, HJ 3373 same star.                                     
01317+6103 STF 128     STI 227.                                                                        
01317+1506 CHR 198     First detected as an occultation binary by Beavers.                     Bvr1977 
01319+1603 BF Psc      Ren & Fu (2013) calculated an astrometric orbit, combining Hipparcos    Ren2013 
                       Intermediate Astrometric Data with spectroscopic elements by                    
                       Griffin (1975).                                                         Grf1975a
01319+1026 GWP 196     XMI 206.                                                                Tob2012b
01320-1604 GAL 310     Object #46 in Gallo's original list.                                    Gal1912a
01321+1657 STF 132     A is a spectroscopic binary, P = 36.6d.                                         
                       A: SB2. Combined orbit including RV data and Hipparcos Intermediate             
                       Astrometric data. Semimajor axis derived from photocentric a0 plus              
                       stellar evolutionary model. Derived properties for A and B:                     
                       M/Msun = 1.14 + 1.02, L/Lsun = 5.40 + 1.41, dm = 1.46 mag,                      
                       log age = 9.86.                                                         WaX2015b
                       AB: H 4 130.                                                            MEv2010 
                       AB, AC, and AD: Optical pairs, based on study of relative motion of             
                       the components using the method of apparent motion parameters.          Kiy2008 
01321+1434 BPM  33     [PM2000]   57016 + [PM2000]   57059.                                    Gvr2010 
01323-2633 ARG   4     B is CD-27@523.                                                                 
01325+1645 BPMA  1     [PM2000]   57224 + [PM2000]   57397.                                    Gvr2010 
01325+1417 LDS1102     NLTT 5103/5102                                                          Chm2004 
01326-2745 LDS2206     NLTT 5136/5135                                                          Chm2004 
01326-4944 SHY 405     HIP   7189 + HIP   7086.                                                        
01327+6336 EVS   9     Primary is the Cepheid V636 Cas.                                        Evs2016a
01327-0139 FIL   2     B is BD-02@235.                                                                 
01328+3551 STF 133     Confusion between C and D in ADS. With quadrant for CD north preceding,         
                       AC obviously has greater separation than AD.                            B__1962d
                       Identifications of several later AC and AD measures were switched to            
                       give motion consistent with earliest measures. Quadrants were flipped           
                       for CD measures, which now agree with AC and AD measures. AC has                
                       smaller separation than AD, and C is slightly brighter than D.                  
           A  1911     Ea,Eb: Originally 01238+3553; found to be E component of 01328+3551.            
01329+1954 LDS3289     NLTT 5133/5127                                                          Chm2004 
01329+1200 GWP 197     XMI 207.                                                                Tob2012b
01329-3652 GC 1881     Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
01330+1027 GWP 198     XMI 208.                                                                Tob2012b
01331-0602 LDS3290     NLTT 5155/5154                                                          Chm2004 
01331-1951 LDS1103     NLTT 5163/5169                                                          Chm2004 
01332+6041 STF 131     Spectrum of B: B3IV.                                                            
01332+3231 SEI  17     Neither component seen on POSS plate; may be flaws on AC Potsdam plate          
01333-0014 UC  582     aka ITF  47.                                                                    
01333-2411 LDS2209     NLTT 5178/5160                                                          Chm2004 
01335+6039 BUP  22     B is BD+59@273.                                                                 
01337-1213 HWE   4     The linear formula by Job & Tamburini seems ruled out, as it makes      Job1969b
                       the current quadrant opposite to what is observed.                              
01343-0827 A   314     Derived orbital parallax 0".00978, mass sum 4.14 +/- 2.34 Msun          Lin2004a
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.85 +/- 0.99, 2.60, and 1.20 Msun, respectively.             Mlk2012 
01344+4844 ES 2587     G172-061. Not a common proper motion companion after comparison with            
                       POSS2 red plates                                                        Oso2004 
01344-1607 FAR  25     Primary is white dwarf WD 0131-163.                                     Far2006 
01345+1448 LDS9119     Old LDS6119.                                                                    
01347+0720 GWP 199     XMI 209.                                                                Tob2012b
01348+2935 BRT   5     An Algol-type system, RS Tri.                                                   
01349+1234 STF 136     AB: H 4 131.                                                            MEv2010 
01349-6909 GLI  12     B is CPD-69@74.                                                                 
01350-2955 BU 1000     AB,C triple+var solution (AB in HIP).                                   Sod1999 
                       B is 0.47d eclipsing binary (= BB Scl).                                         
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
01352-1829 RSS  49     CPD-19@169                                                                      
01354+6305 MLB 280     Also classified K1V.                                                            
01354+4123 ES 1494     Probably identical with ADS 1241 ( = ALD).                                      
01356+6117 STI 237     This and STI 239 are members of the multiple system HJ 1083.                    
01360+2646 BU  507     Morlet et al. note that this has similar position angle, separation,            
                       and delta-m as HDS 212. HDS 212 removed.                                Mor2000 
01360+0739 STF 138     D is BD+06@245.                                                                 
                       AB: H N  92.                                                            MEv2010 
01361-2954 HJ 3447     tau Scl. Arend orbit rejected from Fourth Orbit Catalog                 Ard1968 
                       ("orbit completely faulty and irreparable")                             Wor1983 
01361-3718 HJ 3448     Spectral type of A may be K. B is CD-37@605.                                    
01364+7909 STF 127     B is BD+78@50.                                                                  
01364+3209 SEI  18     Neither component seen on POSS plate; may be flaws on AC Potsdam plate          
                       The faint pair now measured for the lost SEI  18 may be this new pair.  Dam2017a
01368+4124 BUP  23     ups And = 50 And = Titawin. A is a spectroscopic binary.                        
                       AB: exoplanets with P=4.61d, 237.7d, 1302d, 3848d                       Tok2014d
           LWR   1     AD. Determined to be CPM pair from examination of POSS I and II plates          
                       (epochs 1953 and 1995), plus 2MASS. Conclude spectral type of                   
                       companion M4.5V.                                                        Lwr2002 
                       AD: Raghavan et al. (2010) consider D physical, high PM (no PM given).  Rag2010 
           ups And     A: Combined solution, based on reduction of Hipparcos intermediate              
                       astrometric data together with spectroscopic elements from Butler       CPS1999b
                       et al. (1999).                                                          HaI2001 
01372+1147 TOB9002     Measured as HJ   16 but actually an anonymous pair added here.          Tob2010 
                                                                                               Dam2012 
01373+1828 GWP 204     XMI 210.                                                                Tob2012b
01374+2510 G034-039    Boden et al. (2006) give combined spectroscopic/interferometric         Bod2006 
                       solution, including PTI observations. Derive distance of 42.23 +/-              
                       0.21 pc (pi = 23.68 +/- 0.12 mas), age 9.12 +/- 0.25 Gyr, with                  
                       abundances near solar. The K0IV primary appears to have evolved off             
                       the MS and is traversing the Hertzsprung gap toward red giant phase.            
                       Masses are 1.072 +/- 0.014 and 0.8383 +/- 0.0081 Msun, luminosities             
                       2.451 +/- 0.041 and 0.424 +/- 0.023 Lsun, radii 2.048 +/- 0.081 and             
                       0.887 +/- 0.071 Rsun.                                                           
01374-8217 GLI  14     Spectrum G5III:+K1/2.                                                           
01375-1135 LDS9120     Old LDS6120.                                                                    
01376+2233 STTA 20     B is BD+21@218.                                                                 
                       Pair appears in an appendix list, not part of discoverer's regular              
                       numbering sequence.                                                             
01376+1727 GWP 205     XMI 211.                                                                Tob2012b
01376+0709 PLQ  19     HJL  21.                                                                HJL1986 
01376-0645 BRG   5     BC: Initially entered as WDS 01369-0648, the primary of BRG 5 was               
                       later found to be the B component of 01376-0645 CAB 3.                          
01376-0924 KUI   7     1982.7657: This autocorrelogram was remeasured; the new results are             
                       listed here.                                                            McA1987b
                       Combined spectroscopic/visual orbit, also yielding orbital parallax             
                       and component masses and absolute magnitudes.                           Tok1993 
                       Pourbaix gives combined solution for this resolved SB2, yielding                
                       orbital parallaxes and component masses.                                Pbx2000b
                       Martin et al. (1998) derive component masses 1.712 +/- 0.296 and                
                       1.140 +/- 0.226 Msun.                                                   Mig1998 
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.51 +/- 0.43, 2.49, and 1.13 Msun, respectively.             Mlk2012 
01379-8259 TOK 426     HIP 7601 is a nearby (27pc) dwarf also known as GJ 67.1 or HR 512.              
                       According to Wichman et al. (2003 A&A, 400, 293), it is a young                 
                       spectroscopic triple detected in X-rays (1RXS J013755.4-825838). GCS            
                       also recognized the star as SB2. Spectroscopic monitoring (Tokovinin,           
                       in preparation) shows that all three components are similar stars of            
                       approximately one solar mass. Here we resolved the outer subsystem AB           
                       and observed its fast motion. In fact it was already resolved at SOAR           
                       on 2011.036 at 221.0deg and 0".044, but this low-quality observation            
                       has not been published. The available data indicate that the period             
                       of AB is 1.35years; the pair completed nearly two revolutions since             
                       its first resolution in 2011.                                           Tok2015c
01380+4600 HJ 2063     Aka A   944AB,C.                                                                
01385+7302 HJ 2054     40 Cas.                                                                         
01386-4113 CPO 110     B is CD-41@445.                                                                 
01387+0359 GWP 208     XMI 212.                                                                Tob2012b
01387-4515 HJ 3451     LDS  55.                                                                        
01388-1758 LDS 838     LUY 726-8. L 726-8 = UV Cet. Both components are active flare stars             
                       According to Harrington & Behall the mass ratio is 0.487 +/- 0.011 and          
                       the individual masses are 0.115 (0.008) 0.109 (0.008) Msun for A & B,           
                       respectively.                                                           Hrr1973 
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       This pm star with flare characteristics is a difficult object.          VBs1954 
                       Magnitude uncertain due to flares.                                      USN1988b
                       AB: Kervella et al. (2016) derive a new orbit for GJ 65 and determine           
                       the following physical parameters:                                              
                          masses (Msun): A = 0.1225 +- 0.0043   B = 0.1195 +- 0.0043                   
                          radii (Rsun):      0.165  +- 0.006        0.159  +- 0.006                    
                          [Fe/H] (dex):     -0.03   +- 0.20        -0.12   +- 0.20                     
                          log (cgs):         5.092  +- 0.015        5.113  +- 0.015            Krv2016 
01393+1638 BU    5     103 Psc.                                                                        
01394-1748 HJ 2067     HJ 3380.                                                                        
01397+4602 EGB   1     ES 553.                                                                         
01397-3728 HJ 3452     B is CD-38@572.                                                                 
01398+1704 BPM  34     [PM2000]   61379 + [PM2000]   61385.                                    Gvr2010 
01398-5612 DUN   5     Some measures have been corrected by Andrew James (personal                     
                       correspondance). Note that this is p Eri, not rho Eri                           
                       (03027-0741BU   11).                                                            
                       Measures of 1947.60 and 1947.84 made by triangulation of multiple       Der9999 
                       measures.                                                                       
01399+1515 STF 142     B is BD+14@@251.                                                                
01400+2702 ALP   5     2MASSW J0140026+270150                                                          
                       Companion seen as elongated in I-band image taken at WIYN in August             
                       2002. Physical companionship to this ultracool dwarf ruled out.         AlP2007 
01400-1348 GAL 311     Object #48 in Gallo's original list.                                    Gal1912a
01404+3420 STF 143     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
01405-0917 LDS9121     Old LDS6121.                                                                    
01406+4035 BU 1362     tau And = 53 And. A is a spectroscopic binary. Variable?                        
01409+6410 RAO  32     AC: C component = A component of WDS 01409+6409 TDS1951.                        
01409+6409 TDS1951     Primary = C component of WDS 01409+6410.                                        
01409+1117 A  2320     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.33 +/- 0.76, 2.02, and 0.95 Msun, respectively.             Mlk2012 
01409+4952 HU  531     AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 1.66 +/- 0.98, 2.11, and 0.79 Msun, respectively.  Mlk2012 
01409+0138 A  2404     Quadrant uncertain.                                                             
01410-0524 TOK 228     Primary is EY Cet, variable of BY Dra type, X-ray source                Tok2014d
01412-6741 LDS  56     HIP 7869. See Allen et al. (2000) for information on metallicity,       AlC2000 
                       age, galactic orbital parameters, etc.                                          
                       Primary is V773 Cas and SB2, P=1.294d. B at 33.5" 219deg, optical?              
                       CPM according to SIMBAD.                                                Tok2014d
01413+2545 STF 145     Period of AB estimated at 7300y.                                        Tok2006 
                       Primary is SB2, P=4.435d. Aa,Ab has suspected close tertiary because            
                       K1,K2 are var, e>0. B is SB1, P=1.435d.  RoboAO find a companion to B           
                       (98deg, 4.80", dI=7.2mag), but it is considered optical.                Tok2014d
01413+1246 GWP 214     XMI 213.                                                                Tob2012b
01413+1007 STF 146     B is BD+09@203.                                                                 
                       HJL  22.                                                                HJL1986 
01414+3704 LDS3300     NLTT 5619/5621                                                          Chm2004 
01414-7909 HJ 3467     tau 1 Hyi                                                                       
01417+0712 GWP 215     XMI 214.                                                                Tob2012b
01417-7616 JSP  25     Aka TDS1958.                                                                    
01418+4237 MCY   2     An astrometric binary now resolved by infrared speckle interferometry.          
                       Discovery designation per Todd Henry 03/02/98.                                  
                       Improved pc (Delta m > 6) orbit combining pg (Lippincott 1983) and      Lip1983 
                       Hipparcos obs. Scaling by the speckle IR (Henry 1993) gives orbit size  Hen1993 
                       and mass ratio.                                                                 
                       Martin et al. (1998) derive component masses 0.795 +/- 0.159 and                
                       0.136 +/- 0.053 Msun.                                                   Mig1998 
                       The estimated magnitude difference in V (~6 mag) is too large for the           
                       companion to have been detected.                                        Hrt2009 
01419-0907 GRV1170     Aka SLW  81.                                                                    
01420+4252 ROE  64     HJL  23.                                                                HJL1986 
01423+5134 CUD   2     Component A is the central star of the planetary nebula NGC 650/1       Skf2013 
                       = Messier 76.                                                                   
01424+2609 BRT3259     Originally published as BRT 126.                                        Brt1928 
01424-0645 A     1     A premature orbit has been computed.                                            
                       Omega corrected from 24.0 to 58.9, omega from 58.9 to 24.0              Ruy1995 
01425+5000 B  2550     BD+49 440 (8.5) and 441 (9.0) are together in a high power field. Both          
                       are close pairs; brighter star is deep orange, the fainter (ADS 1341,           
                       HU 1210) is white. At present the brighter star is the easier pair,             
                       but as its duplicity was missed by Hussey, Aitken, and van Biesbroeck,          
                       then they measured CD, it must have opened out more recently.           B__1963b
01425+2016 HJ 2071     A: 107 Psc.                                                                     
                       AC: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
           107 Psc     Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
01426+6033 BU 1363     A 3588-d spectroscopic orbit has been found for the A component.        Grf2012d
                       The primary is the E component of 01426+6033.                                   
01427+0637 J  1808     HJL  24.                                                                HJL1986 
01430+6402 STI 264     Component A is a pulsating star in the open cluster NGC 637. Since              
                       relative motions of all three components are small and in agreement             
                       with each other, we believe all three stars are members of the same             
                       cluster. It is not currently possible to determine whether of not they          
                       form a closed triple system.                                            Kiy2012 
01431+3426 COU 668     Aa,Ab: TDS1964.                                                                 
01431+2101 JNN 251     Estimated age 300-1000 Myr; masses 0.30 +/- 0.06 and 0.15 +/- 0.03              
                       Msun; a ~4.8 au.                                                        Jnn2014 
01432+6056 MLR 106     AC: STI 271.                                                                    
01433+6033 BU 1103     44 Cas. A is a spectroscopic binary.                                            
           FYM 160     AH: Fay (2013) notes an H component in their Figure 1, but does not     FyM2013d
                       include a measurement.                                                          
           ARN  32     AE: E component is primary of 01426+6033 BU 1363                                
01433-1736 HJ 3455     B is BD-18@292.                                                                 
01434-0705 STF 150     B is BD-07@283.                                                                 
01434-1127 GAL 312     Object #50 in Gallo's original list.                                    Gal1912a
01435+5318 HJ 2069     B is BD+52@417.                                                                 
01435-1038 GAL 313     Object #51 in Gallo's original list.                                    Gal1912a
01436+2802 GIC  24     G072-028/G072-029.                                                              
                       NLTT 5738/5740                                                          Chm2004 
01437+5014 CIA   6     Phi Per. Be+sdO binary, resolved by the CHARA Array. The hot subdwarf           
                       companion is detected in near-IR; flux contribution 1.5% in H (dH=4.6)          
                       and restricted fits indicate flux contribution rises to 3.3% (dV~3.7)           
                       in visible.  Combined interferometric/spectroscopic orbital solution            
                       yields masses 9.6+/-0.3 and 1.2+/-0.2 Msun for the Be primary and               
                       subdwarf secondary, respectvely. The inferred distance (186+/-3pc),             
                       kinematical properties, and evolutionary state are consistent with              
                       membership of phi Per in the alpha Per cluster.                         CIA2015a
01437+0934 BU  509     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.69 +/- 0.64, 1.83, and 0.85 Msun, respectively.             Mlk2012 
01438+1954 GWP 216     XMI 215.                                                                Tob2012b
01438+1206 HJ   18     Possibly BD+11@225. BDS 899, HJ 18. HJ position angle in 1820: 220@.            
                       Disagrees with 1912 - 1922: 143@.                                               
01441-1556 BUP  25     tau Cet = 52 Cet. Optical. Proper motion of A -1718 +856.                       
01442-0813 LDS9122     Old LDS6122. Primary is QSO, Z=0.239.                                           
01443+6652 HAU  10     HJL  25.                                                                HJL1986 
01443+5732 BU  870     A premature orbit has been computed.                                            
                       Primary is eclipsing binary V773 Cas (period 2.58734 day).              Zas2010 
                       Light curve and radial velocity combined solution determined.           Zas2017 
           ARN  55     AD: HJL1011.                                                            HJL1986 
01443+0929 KPR   1     AC: Separation may be a factor of 10 too small.                                 
           STF 155     AB: H 2  49.                                                            MEv2010 
01448+5708 B  2548     Rapid motion.                                                                   
                       This close pair precedes BD+56 338 (ADS 1371, BU 453) by 12 sec of              
                       time and is 0.6' north of it. All measures given in Pub Yerkes O. IX,           
                       pt 1 and 2, by van Biesbroeck and myself, assigned to BU 453, are               
                       obviously of the new pair. My estimates of the difference in magnitude          
                       vary between 0.4 sf and 0.7 np, which seems rather large to be error            
                       of estimation, even in so close a pair.                                 B__1963b
01449+2005 109 Psc     Combined solution, based on reduction of Hipparcos intermediate                 
                       astrometric data together with spectroscopic elements from Vogt et al.  CPS2000c
                       (2000).                                                                 HaI2001 
01449+1951 A  2322     EU Psc, Algol (EA) type eclipsing binary,  per 1.69261 d.               Zas2011 
                       Observed wrong star? van den Bos has 4 measures in 1962, and I have     B__1963b
                       positive measure in 1964.                                               Wor1967b
01450+6032 STI 281     AB: BKO1073AC.                                                                  
           MRI  27     AC: BKO1073AB.                                                                  
01450+5707 BU  453     Premature orbits have been calculated. Motion direct.                   Baz1972 
01450+2703 COU 750     Rapid motion.                                                                   
01450-0104 LDS9123     Old LDS6123.                                                                    
                       NLTT 5822/5818                                                          Chm2004 
01452+2317 GIC  25     G034-048/G034-049.                                                              
01454+0909 OCC9041     110 omi Psc.                                                                    
01454-3957 BRG   6     2MASS J01452133-3957204 has only been observed in one epoch, but the            
                       color and brightness of the detected companion are consistent with              
                       expectation, hence we count it as an unconfirmed binary.                Jnn2012 
01455-6035 JSP9001     Previously known as JSP  13a.                                                   
01456+1148 GWP 217     XMI 216.                                                                Tob2012b
01456-0224 J  1448     BC. Gauchet (1926) measure originally listed as CD pair, with theta     Gau1926a
                       flipped by 180deg.                                                              
01456-2503 HJ 3461     eps Scl. A premature orbit has been computed.                                   
01457+0834 BAG  38     Primary is the alpha2 CVn type variable UZ Psc.                                 
01458+1200 BPM  35     [PM2000]   64864 + [PM2000]   64876.                                    Gvr2010 
01458+0043 GWP 219     XMI 217.                                                                Tob2012b
01459+7142 HJ 1090     01459+7142FOX 119CD. WDS designation for HJ 1090 changed from                   
                       01461+7143 due to inclusion in multiple.                                        
01459-4357 HJ 3463     B is CD-44@509.                                                                 
01460+8005 GW Cep      Multiple system including contact binary.                               Pbl2006 
01460+6113 STF 151     STF 151rej and Duner 1 are identical.                                           
01462+5326 HJ 2079     Confused with nearby 01463+5328 HJ 2080, as pairs are also of similar           
                       separation and position angle.                                                  
01462+3343 HU  804     A premature orbit has been computed.                                            
01463+5328 HJ 2080     Confused with nearby 01462+5326 HJ 2079, as pairs are also of similar           
                       separation and position angle.                                                  
01466+1639 GWP 221     XMI 218.                                                                Tob2012b
01467+0214 GWP 222     XMI 219.                                                                Tob2012b
01469+4234 DUP   1     Dupuy et al. (2015) resolved a low-luminosity T9/Y0 binary, using Keck          
                       laser guide star imaging. Masses are estimated as 4.6 +1.0/-1.1 and             
                       4.3 +1/0/-1.2 Mjup (for age of 1Gyr) or 16.9 +3.8/-4.0 and                      
                       15.9 +3.5/-4.4 Mjup  (for age of 10Gyr).                                Dup2015 
01474+0355 HJ 2084     Aka STT  36.                                                                    
01474-2157 GD 1400     Song et al. (2006) confirm common proper motion of this brown dwarf     Son2006 
                       and its planetary mass companion.                                               
01475-4955 RED  15     2MASS J01473282-4954478. Spectral types M8: and L2:                     Red2006b
01476+3453 CSW   1     AB: This star has a possible wide brown dwarf companion at 43"          Csw2008 
                       separation, according to Casewell et al. (2008).                        Jnn2012 
           KIR   6     BC: B component is an L0.5V brown dwarf. The spectrum of the secondary          
                       shows it to be a background M star.                                     Kir1999 
01477+6351 ENG   7     A is GJ 75 = V987 Cas. B is BD+63@241.                                          
01477+1643 BPMA  2     [PM2000]   65958 + [PM2000]   65844.                                    Gvr2010 
01477-4358 I    52     Gomez et al. (2016) derive dynamical parallax and component masses:             
                       7.50 +/- 0.33 mas, 1.310 +/- 0.032 Msun, 1.128 +/- 0.027 Msun.          Doc2016i
01478-8011 HJ 3474     tau 2 Hyi                                                                       
01479+4440 A   949     BJN  26.                                                                        
                       This measure was published as BRT 346. Note to BRT 346: This seems to           
                       be ADS 1412, although the magnitude difference is discordant.                   
                       BD+44  369, with which ADS 1412 is identified, was not seen as double.  Brt1939a
01480+4353 ES 1498     BRT 325.                                                                Brt1930 
01481-2533 FAR  26     Primary is white dwarf WD 0145-257.                                     Far2006 
01483+1203 LDS1116     LDS3311.                                                                        
                       NLTT 6012/6013                                                          Chm2004 
01483-4130 RGS   2     GJ 77. Rodigas et al. (2016) detect a companion to the old solar-type           
                       star HD 11112, and determine it is likely a gravitationally bound cool          
                       white dwarf. SED fits (pure-H and pure-He models) suggest a mass for            
                       the companion in the range 0.90-1.08 Msun, Teff 7300-9800K,                     
                       log (L/Lsun) -3.69 - -3.36, and age 2.43-3.92 Gyr.                      Rgs2016b
01486+1618 BU  510     AC: H 5  92.                                                            MEv2010 
01486-0955 JNN  17     LP 708-465.                                                                     
01487+7528 HJ 2075     LDS1540.                                                                        
01487+3306 GIC  26     G072-038/G072-037.                                                              
                       NLTT 6030/6027                                                          Chm2004 
01487-2916 HJ 3466     B is CD-29@590.                                                                 
01488-0125 STF 171     B is BD-02@300.                                                                 
01489+1411 GWP 223     XMI 220.                                                                Tob2012b
01489-2053 ARA1256     Primary is TW Cet, a W UMa type eclipsing binary, P = 0.31685d.         Zas2012 
01489-3153 LDS3316     NLTT 6087/6088                                                          Chm2004 
01491+0236 GWP 224     XMI 221.                                                                Tob2012b
01493+4754 CHR   4     Aa,Ab: Although this new component is indicated as Aa,Ab we have not            
                       firmly established whether it is associated with the A or B component           
                       of the wide pair.                                                       McA1987b
                       B is a spectroscopic binary. The system appears to be quintuple.                
01493+1808 GWP 225     XMI 222.                                                                Tob2012b
01496+1741 GWP 226     XMI 223.                                                                Tob2012b
01496-1041 ENG   8     53 Cet = chi Cet. LDS2222.                                                      
                       SHY   8. Bayesian analysis by Shaya & Olling (2011) indicates very      Shy2011 
                       high (near 100%) probability pair is physical.                                  
01497-1414 HU  422     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 1.42 +/- 0.46, 2.45, and 1.20 Msun, respectively.             Mlk2012 
01498-3824 GC 2219     Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
           HDO 186     Additional notes may be found in Herschel (1847).                       HJ_1847b
01499+8053 STT  34     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 14.28 +/- 6.95, 4.72, and 2.24 Msun, respectively.            Mlk2012 
01499+1324 LDS1118     Also known as LDS6124 and LDS9124. Richard Jaworski first               Jaw2006 
                       recognized that these systems were the same.                                    
01500-0408 A  2602     Gomez et al. (2016) derive dynamical parallax and component masses:             
                       15.65 +/- 1.62 mas, 0.748 +/- 0.037 Msun, 0.748 +/- 0.037 Msun.         Doc2016i
01501+3538 ALI  28     No stars seen at AC catalog locations - probably plate flaws.                   
01501+2217 STF 174     1 Ari. Spectrum composite; K1III+A6V. Spectroscopic binary?                     
                       H 1  73.                                                                MEv2010 
01502+1600 BPM  36     [PM2000]   67462 + [PM2000]   67449.                                    Gvr2010 
01503+1146 GWP 227     XMI 224.                                                                Tob2012b
01504+2942 MLB1059     Aka MLB 448.                                                                    
01509+1626 BPM  37     [PM2000]   67854 + [PM2000]   67921.                                    Gvr2010 
01509+1031 GWP 228     XMI 225.                                                                Tob2012b
01510+2107 STF 175     AB: H 2  56.                                                            MEv2010 
01511+1135 BPM  38     [PM2000]   68017 + [PM2000]   67969.                                    Gvr2010 
01512+2439 HO  311     Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 4.19 +/- 1.30, 3.38, and 1.40 Msun, respectively.             Mlk2012 
01513+6451 STF 163     B is BD+64@244.                                                                 
01513-3800 LDS9125     Old LDS6125.                                                                    
01514+4329 HJ 2089     B is BD+42@388.                                                                 
01515+0457 STF 177     Formerly, BD+04@320. Corrected by Weis.                                         
01515-0744 HIP   8653  Small acceleration of 2 mas yr-2, possibly single.                      Tok2012a
01515-1020 BNU   1     Aa,Ab: zet Cet = 55 Cet = Baten Kaitos. A is a long-period                      
                       spectroscopic binary, P = 1652d, and has been resolved by speckle               
                       interferometry. B is BD-11@360.                                                 
01515-1858 LDS9126     Old LDS6126.                                                                    
01516+1618 BPM  39     [PM2000]   68302 + [PM2000]   68249.                                    Gvr2010 
01518-5458 SHY 128     AC: HIP   8687 + HIP   7387.                                                    
01519+6426 GIC  27     G244-037/G244-036 = GJ 3117A/3118B.                                             
01520+1049 STF 178     H 1  56.                                                                MEv2010 
                       Additional notes may be found in Couteau (1952).                        Cou1952a
01521+5430 SMA  24     Also known as STI1703.                                                          
01522+6627 STF 167     Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
01522-5220 CVN   3     CPM pair. The spectral type of the B component is M9.5 +/- 1,                   
                       Teff = 2100 +/- 200K; age ~30 Myr, mass 25 +/- 10 Mjup.                 Cvn2005a
01523-0620 LDS9127     Old LDS6127.                                                                    
01525+1710 GWP 232     XMI 226.                                                                Tob2012b
01526+3127 HJ  645     SEI  20.                                                                Nsn2017a
01528+4016 MLB 999     BRT 2198.                                                                       
01528+1544 BPM  40     [PM2000]   69032 + [PM2000]   69018.                                    Gvr2010 
01528+0117 GWP 233     XMI 227.                                                                Tob2012b
01530-2805 HJ 3472     SWR   3. CPM pair                                                       Skf2004 
01531+2935 BUP  27     alp Tri = 2 Tri = Mothallah. A is a spectroscopic binary, P = 1.77d.            
01532+3719 STF 179     H 1  89.                                                                MEv2010 
01533+4044 HJ 1094     55 And.                                                                         
01534+7003 STF 169     Primary is V776 Cas, a W UMa type eclipsing binary, P = 0.44042d.       Zas2012 
01535+1918 STF 180     gam Ari = 5 Ari = Mesarthim. According to R.G. Aitken, Robert Hooke     A__1935f
                       noted this as a double in 1664. Hooke wrote: "I took notice that it     Hoo1665 
                       consisted of two small stars very near together; a like instance to             
                       which I have not else met in all the heavens."                          HFC1928 
                       A is a variable of the Alpha CVn type.                                          
                       AB: H 3   9.                                                            MEv2010 
           BU  512     Primary is C component of STF 180. WDS designation changed from                 
                       01538+1918 and components labelled CD.                                          
01536+6324 PTT   3     OL 114, STI 317 are identical.                                                  
01536+0311 xi Psc      Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Griffin & Herbig (1981).                                                Grf1981b
01541-7729 JSP  31     Apparent rapid retrograde motion, but measures sparse.                          
01543+6542 GIC  28     G244-042/G244-041.                                                              
01543-1543 GAL 314     Also known as LDS1120.                                                          
                       Object #55 in Gallo's original list.                                    Gal1912a
                       Optical pair, based on study of relative motion of the components               
                       using the method of apparent motion parameters.                         Kiy2008 
           CHM   3     AC. NLTT 6398 + 6395.                                                           
01544-2250 LDS3322     NLTT 6400/6399                                                          Chm2004 
01544-4230 phi Phe     Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
                       Chemically peculiar late-B star, initially thought to be a triple,              
                       with spectroscopic period 41.4d and astrometric period 878d. Using              
                       Coralie spectra from 2000-2010, Korhonen et al. (2013 A&A 553, A27)             
                       find a spectroscopic period of 1126d. Spectroscopic data by Pourbaix            
                       et al. (2013) exclude the 40d period, but are insufficient to refine            
                       the Korhonen solution. Their spectroscopic elements are combined                
                       with the Hipparcos astrometry to refine the initial astrometic orbit.   Pbx2013 
01546+2049 MKT   3     bet Ari = Sheratan. Astrometry from Mark III interferometer is combined         
                       with spectroscopy (Tomkin & Tran 1987) by Pan et al. (1990) to          Tom1987b
                       determine orbital elements, masses, and distance. Masses agree well     MkT1990 
                       with empirical mass-luminosity relation.                                        
                       Hipparcos astrometric solution adopted some elements from the orbit of  HIP1997d
                       Pan et al. (1990).                                                      MkT1990 
                       Martin et al. (1998) derive component masses 2.067 +/- 0.203 and                
                       1.281 +/- 0.178 Msun.                                                   Mig1998 
                       Pourbaix gives combined solution for this resolved SB2, yielding                
                       orbital parallaxes and component masses.                                Pbx2000b
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 3.19 +/- 0.13, 3.51, and 1.82 Msun, respectively.             Mlk2012 
01549+1124 BPM  41     [PM2000]   70299 + [PM2000]   70233.                                    Gvr2010 
01551+2847 STF 183     According to Scardia et al. (2001), orbital elements are well defined;  Sca2001d
                       only the period is still rather uncertain. The Hipparcos parallax               
                       (0".00727 +/- 0.00189) gives a mass sum of 3.8 Msun +/- 82%, in excess          
                       for a binary of type F2. The dynamical parallax (0".0074) agrees well           
                       with the observed one.                                                          
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 4.82 +/- 2.85, 3.45, and 1.35 Msun, respectively.  Mlk2012 
01551-1204 LDS9128     Old LDS6128.                                                                    
01553-2134 DON  26     CD-22@641.                                                                      
01554+0257 A  2407     A premature orbit has been computed.                                            
01556+0146 BU 1367     A 2408.                                                                         
01559+0151 STF 186     Spectroscopic binary?  Spectrum composite; F7V+G0V.                             
                       See Baize & Petit (1989) catalog of doubles with variable component.    Baz1989d
                       Malkov et al. (2012) derive dynamical, photometric, and spectroscopic           
                       masses of 2.22 +/- 1.22, 2.56, and 1.07 Msun, respectively.             Mlk2012 
01560+0529 GWP 236     XMI 228.                                                                Tob2012b
01560+0046 RST5186     BD+00@311a.                                                                     
01560-5137 HJ 3473     chi Eri                                                                         
01561+6035 AG  301     HJL  26.                                                                HJL1986 
01561+3745 HJ 1097     ALI 494.                                                                        
01562+3715 BU 1368     Bb: b is BD+36@349.                                                             
           STFA  4     56 And. B is BD+36@354.                                                         
01563+0829 GWP 237     AB: XMI 229AB.                                                          Tob2012b
           GWP 238     AC: XMI 229AC.                                                          Tob2012b
01564+3650 J  2719     ALI 259.                                                                        
01568+3931 ALI1022     Not found by Heintz at IDS position.                                    Hei1990b
01568+3802 TOB9001     BC: A measure by Espin incorrectly attributed to this pair led to its           
                       earlier designation as 01569+3759ES  228CD.                                     
01568+2303 BVD  21     RoboAO resolved the B component (201.1deg, 0.199", dI=1.61 mag) but             
                       the pair was not accepted as real.                                      Tok2014d
01570+3101 A   819     A premature orbit has been computed.                                            
                       AB: Malkov et al. (2012) derive dynamical, photometric, and                     
                       spectroscopic masses 1.97 +/- 1.00, 2.49, and 1.20 Msun, respectively.  Mlk2012 
                       AB,C: HJL  27.                                                          HJL1986 
01571+1517 BPM  43     [PM2000]   71640 + [PM2000]   71653.                                    Gvr2010 
01571+1414 BPM  42     [PM2000]   71596 + [PM2000]   71608.                                    Gvr2010 
01572+1644 GWP 241     XMI 230.                                                                Tob2012b
01572-1015 GAL 315     LDS  60. Object #56 in Gallo's original list.                           Gal1912a
                       HIP 9094. See Allen et al. (2000) for information on metallicity,       AlC2000 
                       age, galactic orbital parameters, etc.                                          
                       NLTT 6529/6530                                                          Chm2004 
01575+5558 ES 1811     STI1732.                                                                        
                       Vatican zone coordinates yield 1911.9, 295.2, 5.61, showing Espin's             
                       distance is too small and that there is no change so far.               VBs1954 
01576+4205 YSC 125     There is some evidence of a very faint third component in this system           
                       with separation of 0.45 arcsec.                                         Hor2011b
           NLTT 6522   Orbit determined by fitting revised Hipparcos intermediate astrometric          
                       data. Derived component masses 0.99 +/- 0.11 and 0.75 +/- 0.05 Msun.    Ren2010 
01577-3625 LDS  62     LDS5359. TSN  72.                                                               
01579+2336 H 5  12     H V 12. STTA 21. 9 Ari = lam Ari. A is a Beta Lyrae-type and                    
                       spectroscopic binary.  B is BD+22@289.                                          
                       AB: HJL  28.                                                            HJL1986 
01579+0924 GWP 243     XMI 231.                                                                Tob2012b
01579-2851 LDS  61     NLTT 6581/6583                                                          Chm2004 
01581+4123 S   404     Same as STF 190 rej, SHJ 404, H IV 104, H 4 104, H IV 128, H 4 128.             
                       AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
01583+0250 GWP 245     XMI 232.                                                                Tob2012b
01583-8218 I   311     Composite spectrum: G8/K0(V)+(G).                                               
01584+2547 A  2011     B is strongly above MS, very red in V-K (wrong 2MASS ptm?). Hipparcos           
                       does not resolve AB, but has X-solution and suspected non-single.       Tok2014d
01584-2304 LDS3330     NLTT 6605/6606                                                          Chm2004 
01585+3643 J  1809     ALI 262.                                                                        
01586+3834 LPL   1     La Palombara et al. (2012) detect a companion to the hot subdwarf               
                       BD+37 442, using the XMM Newton satellite. The companion is thought to          
                       be a white dwarf or neutron star, likely powered by accretion from the          
                       wind of the primary.                                                    LPl2012 
01586-5332 HU 1557     Primary is CI Eri, an Algol type eclipsing binary, P = 1.23819d.        Zas2012 
01588+1702 GWP 247     XMI 233.                                                                Tob2012b
01588-0949 J  1449     BD-10  410. Previously published declination corrected by +4'.          J__1949a
                       GAL 316. Object #57 in Gallo's original list.                           Gal1912a
01588-2212 HJ 2103     B is BD-22@329.                                                                 
01588-6134 alf Hyi     Hipparcos astrometric solution assumed circular orbit (e = omega = 0)   HIP1997d
01589-5652 LDS  63     LDS6106 = LDS9106 (incorrectly listed in the WDS as 00593-5652).                
                       B is CPD-57@385 = CD-57@396.                                                    
01590-1640 LDS9129     Old LDS6129.                                                                    
01590-2255 H 2  58     H II 58. A is a W UMa-type system, AA Cet.                                      
01591+3313 ENG   9     AB: Optical pair, based on study of relative motion of the components           
                       using the method of apparent motion parameters.                         Kiy2008 
01591+1523 GWP 248     XMI 234.                                                                Tob2012b
01598+1543 BPM  44     [PM2000]   73241 + [PM2000]   73209.                                    Gvr2010