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Table 3:

The rejected PSR.

PSR  		l b DM D $RM\pm\Delta RM$ $I_{\rm H\alpha}$ H$\alpha$ HII-region SNR $D_{\it SNR}$  
  deg deg pc/cm3  kpc rad/m2 R step  RCW nr. D(kpc)    kpc

J0831-4406 		262.28 -2.69 254 0.47 509 $\pm$ 20 102 3 Gum Neb.   G263.9-3.3 0.31
J0835-4510 263.55 -2.79 68 0.24 30 $\pm$ 1 98 1     G263.9-3.3 0.31,2
J0855-4644 266.96 -1.00 238 3.88 249 $\pm$ 22 100 2 Gum Neb. 0.43,4 G266.2-1.2 0.255
J0855-4658 267.11 -1.19 473 12.81 350 $\pm$ 50 120 2 Gum Neb. 0.43,4 G266.2-1.2 0.255
J0955-5304 278.30 1.20 157 4.86 -97 $\pm$ 13 28       G279+1.1 36
J1012-5857 283.70 -2.14 384 7.93 72 $\pm$ 8 75 2 47 3.27    
J1019-5749 283.83 -0.67 1039 6.94 -366 $\pm$ 10 159 1 49 4.78    
J1016-5857 284.07 -1.88 394 8.00 -537 $\pm$ 17 105 2 47 3.27    
J1049-5833 287.62 0.64 447 7.64 359 $\pm$ 11 89 3 53 2.79    
J1043-6116 288.22 -2.10 449 9.46 257 $\pm$ 23 147 2 54 3.110    
J1054-5943 288.72 -0.10 331 5.78 46 $\pm$ 34 157 3 53,54 2.79, 3.110    
J1103-6025 289.99 -0.29 276 4.99 569 $\pm$ 7 139 3 54 3.110    
J1105-6107 290.49 -0.85 271 4.98 187 $\pm$ 1 156 1 54 3.110    
J1112-6103 291.22 -0.46 599 12.24 242 $\pm$ 15 675 1 54, 57B 3.110, 7.98    
J1117-6154 292.10 -1.02 494 8.91 -622 $\pm$ 10 80 3 57B 7.98    
J1119-6127 292.15 -0.53 707 17.14 832 $\pm$ 6 127 3 57B 7.98 G292.2-0.5 8.411
J1123-6259 293.18 -1.78 223 4.28 54 $\pm$ 10 64 3 60 2.212    
J1133-6250 294.21 -1.29 568 12.1 848 $\pm$ 6 300 2 62 2.212    
J1138-6207 294.50 -0.46 520 9.65 594 $\pm$ 18 95 2 62 2.212    
J1305-6455 304.41 -2.09 505 12.09 -420 $\pm$ 5 83 2 74 3.813    
J1305-6203 304.56 0.77 470 8.51 -436 $\pm$ 15 73 2 74 3.813    
J1317-6302 305.90 -0.32 678 12.06 -504 $\pm$ 8 179 1 74 3.813    
J1324-6146 306.85 0.85 828 10.12 -1546 $\pm$ 29 75 214        
J1341-6220 308.73 -0.04 730 8.66 -900 $\pm$ 40 55       G308.7+0.0 6.915
J1406-6121 311.84 0.20 542 8.15 880 $\pm$ 60 73 2 83 1.5;1.316    
J1413-6222 312.24 -0.98 808 15.51 -490 $\pm$ 8 74 2 83 1.5;1.316    
J1412-6145 312.32 -0.36 515 7.82 -39 $\pm$ 20 94 1 83 1.5;1.316    
J1413-6141 312.46 -0.33 677 10.14 -35 $\pm$ 10 72 2 83 1.5;1.316    
J1452-5851 318.08 0.39 262 4.3 47 $\pm$ 7 18       G318.2+0.1 <117
J1513-5908 320.32 -1.16 253 4.21 216 $\pm$ 1 133 2 89 316    
J1635-4944 335.39 -1.57 474 6.62 -23 $\pm$ 15 77 3 108 1.318    
J1628-4804 335.76 0.46 952 9.79 -431 $\pm$ 43 120 2 108 1.318    
J1632-4818 336.08 -0.20 758 7.77 -515 $\pm$ 39 102 3 108 1.318    
J1630-4733 336.40 0.56 498 5.65 -348 $\pm$ 6 96 2 108 1.318    
J1630-4719 336.49 0.78 490 5.79 -339 $\pm$ 10 68 2 108 1.318    
J1640-4715 337.71 -0.43 592 6.48 -411 $\pm$ 12 87 2 108 1.318    
J1644-4559 339.19 -0.20 479 5.09 -617 $\pm$ 1 91 319        
J1639-4359 340.02 1.87 259 4.02 129 $\pm$ 18 57 3 113 2.220    
J1646-4346 341.10 0.96 490 5.79 -24 $\pm$ 18 201 2 113 2.220 G341.2+0.921  
J1649-4349 341.36 0.59 399 5.02 759 $\pm$ 17 205 1 113 2.220    
J1651-4246 342.45 0.92 525 6.35 -154 $\pm$ 5 112 3 113 2.220    
J1653-4249 342.63 0.62 416 5.24 25 $\pm$ 17 160 2 113 2.220    
J1709-4429 343.10 -2.69 76 2.3 -7 $\pm$ 4 33       G343.1-2.3 321,22
J1701-3726 347.75 2.83 303 5.17 -606 $\pm$ 8 136 2 119 1.723    
J1715-3903 348.10 -0.32 313 4.11 250 $\pm$ 15 92 2 119,123 1.723, 3.324    
B1718-35 351.69 0.67 496 5.8 159 $\pm$ 4 75 2 127 1.725    
J1717-3425 352.12 2.02 588 9.98 -191 $\pm$ 14 102 2 130 18    

Notes.  (1) Parallax dist., Caraveo et al. (2001) (Vela remnant); (2) ``Vela PSR'' (B0833-45) associated with Vela remnant; (3) Mitra & Ramachandran (2001); (4) kinematic/stellar dist., Sahu (1992); (5) parallax Cha et al. (1999); (6) $\Sigma$-D dist., Duncan et al. (1995a); (7) stellar dist., Avedisova & Palous (1989); (8) kinematic dist., Russeil (2003); (9) stellar dist., Tapia et al. (2004); (10) assoc. with HI-shell, radial vel., Rizzo & Arnal (1998); (11) HI abs., kinematic dist., Caswell et al. (2004); (12) kinematic dist., Georgelin et al. (2000); (13) stellar dist. (HII-region part of extended star formation complex with several HII-regions), Georgelin et al. (1988); (14) HII-region G307.1+1.2 close to line-of-sight (likely to be in front of PSR), Cordes & Lazio (2003, Paper II); (15) $\Sigma$-D dist., Kaspi et al. (1992); (16) kinematic/stellar dist., Georgelin et al. (1987); (17) X-ray emission, Bocchino et al. (2001); (18) CO velocities, Arnal et al. (2003); (19) several HII-regions with distances compatible with being in front of PSR, Cordes & Lazio (2003, Paper II); (20) kinematic dist., Georgelin et al. (1996); (21) possible assoc. PSR wind and nebula, Giacani et al. (2001); (22) although inaccurate $\Sigma$-D dist. places SNR beyond PSR, likely assoc. PSR and SNR, Dodson & Golap (2002); (23) stellar dist. and association with HI shell, Benaglia & Cappa (1999); (24) UBVRI photometry, Vazquez & Baume (2001); (25) CO velocities, Blitz et al. (1982).


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