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Table D.1

Master list of the pulsars used in our study.

B-name J-name l b ϖ ′ σ ϖ σ α σ δ τ c Ref.
(°) (°) (mas) (mas/yr) (mas/yr) (Myr)
1 J0034−0721 110.42 −69.82 0.93 0.08 10.37 0.08 −11.13 0.16 36.7 6
2 J0108−1431 140.93 −76.82 4.17 1.42 75.05 2.26 −152.54 1.65 166.4 5
3 B0136+57 J0139+5814 129.22 −4.04 0.37 0.04 −19.11 0.07 −16.60 0.07 0.4 6
4 B0329+54 J0332+5434 i 145.00 −1.22 0.94 0.11 17.00 0.27 −9.48 0.37 5.5 1
5 B0355+54 J0358+5413 i 148.19 0.81 0.91 0.16 9.20 0.18 8.17 0.39 0.6 4
6 B0450+55 J0454+5543 152.62 7.55 0.84 0.05 53.34 0.06 −17.56 0.14 2.3 6
7 J0538+2817 i 179.72 −1.69 0.72 0.12 −23.57 0.10 52.87 0.10 0.6 6
8 B0628–28 J0630−2834 236.95 −16.76 3.01 0.41 −46.30 0.99 21.26 0.52 2.8 5
9 B0656+14 J0659+1414 i 201.11 8.26 3.47 0.36 44.07 0.63 −2.40 0.29 0.1 2
10 B0809+74 J0814+7429 140.00 31.62 2.31 0.04 24.02 0.09 −43.96 0.35 122.0 1
11 B0818–13 J0820−1350 235.89 12.59 0.51 0.04 21.64 0.09 −39.44 0.05 9.3 6
12 B0919+06 J0922+0638 225.42 36.39 0.83 0.13 18.35 0.06 86.56 0.12 0.5 3
13 B0950+08 J0953+0755 228.91 43.70 3.82 0.07 −2.09 0.08 29.46 0.07 17.5 1
14 B1133+16 J1136+1551 241.90 69.20 2.80 0.16 −73.95 0.38 368.05 0.28 5.0 1
15 B1237+25 J1239+2453 252.45 86.54 1.16 0.08 −106.82 0.17 49.92 0.18 22.9 1
16 B1508+55 J1509+5531 91.33 52.29 0.47 0.03 −73.64 0.05 −62.65 0.09 2.3 6
17 B1541+09 J1543+0929 17.81 45.78 0.13 0.02 −7.61 0.06 −2.87 0.07 27.5 6
18 B1556–44 J1559−4438 334.54 6.37 0.38 0.08 1.52 0.14 13.15 0.05 4.0 5
19 B1929+10 J1932+1059 i 47.38 −3.88 2.78 0.06 94.06 0.09 43.24 0.17 3.1 7
20 J1935+1616 52.44 −2.09 0.22 0.12 1.13 0.13 −16.09 0.15 0.9 6
21 B2016+28 J2018+2839 68.10 −3.98 1.03 0.10 −2.64 0.21 −6.17 0.38 59.8 1
22 B2020+28 J2022+2854 68.86 −4.67 0.61 0.08 −3.46 0.17 −23.73 0.21 2.9 7
23 B2021+51 J2022+5154 87.86 8.38 0.78 0.07 −5.03 0.27 10.96 0.17 2.7 7
24 B2045–16 J2048−1616 30.51 −33.08 1.05 0.03 113.16 0.02 −4.60 0.28 2.8 6
25 B2053+36 J2055+3630 79.13 −5.59 0.17 0.03 1.04 0.04 −2.46 0.13 9.5 6
26 J2144−3933 i 2.79 −49.47 6.05 0.56 −57.89 0.88 −155.90 0.54 272.3 5
27 B2154+40 J2157+4017 90.49 −11.34 0.28 0.06 16.13 0.10 4.12 0.12 7.1 6
28 B2310+42 J2313+4253 104.41 −16.42 0.93 0.07 24.15 0.10 5.95 0.13 49.3 6

Notes. The last column gives the reference in Table 2 from which the parallax with error (Cols. 7, 8), and the proper motions with their errors (Cols. 9–12) are taken. In the case of asymmetric errors we take the larger one. Columns 11 gives the characteristic age τc ≡ P/ (2Ṗ). An i in Col. 5 indicates that the model velocity distribution for this pulsar is isotropic in the models that mix isotropic and semi-isotropic velocity distributions.

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