Table 3
Proper motion and parallax measurements for the pulsars considered in this study.
| Pulsar | PMRA (mas yr-1) | PMDEC (mas yr-1) | PMTOT (mas yr-1) | PX (mas) | Derived PX distance (kpc) | References | |||||
| This work | Prev. | This work | Prev. | This work | Prev. | This work | Prev. | This work | Prev. | ||
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|
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| J0034−0534 | 7.9(8) | – | −9.9(17) | – | 12.6(14) | 31(9) | <7.4 | – | >0.14 | – | –, –, 1, – |
| J0340+4130 | −0.59(16) | – | −3.81(34) | – | 3.85(33) | – | <1.3 | – | >0.77 | – | –, –, –, – |
| J0610−2100 | 9.21(6) | 7(3) | 16.73(8) | 11(3) | 19.10(8) | 13(3) | <1.3 | – | >0.77 | – | 2, 2, 2, – |
| J0614−3329 | 0.58(9) | – | −1.92(12) | – | 2.00(11) | – | <2.2 | – | >0.45 | – | –, –, –, – |
| J0740+6620 | −6(11) | – | −32(4) | – | 32.6(41) | – | <11.7 | – | >0.09 | – | −, –, –, – |
| J0751+1807 | −2.71(7) | – | −13.2(4) | – | 13.51(35) | 6.0(20) | 0.66(15) | 1.6(8) | 1.51(35) | 0.62(31) | −, –, 3, 3 |
| J0931−1902 | −1.1(8) | – | −4.4(12) | – | 4.6(12) | – | <5.0 | – | >0.20 | – | −, –, –, – |
| J1024−0719 | −35.247(23) | −35.3(2) | −48.14(5) | −48.2(3) | 59.67(4) | 59.7(3) | 0.89(14) | 1.9(8) | 1.13(18) | 0.53(22) | 4, 4, 4, 5 |
| J1231−1411 | −62.03(26) | −100(20) | 6.2(5) | −30(40) | 62.34(26) | 104(22) | <1.8 | – | >0.56 | – | 6, 6, 6, – |
| J1455−3330 | 7.88(5) | 5(6) | −1.90(12) | 24(12) | 8.11(5) | 25(12) | 0.99(22) | – | 1.01(22) | – | 7, 7, 7, – |
| J1614−2230 | 3.87(12) | – | −32.3(7) | – | 32.5(6) | 32(3) | 1.30(9) | 0.5(6) | 0.77(5) | 2.0(24) | −, –, 8, 9 |
| J1730−2304 | 20.7(4) | 20.27(6) | 8.3(83) | – | 22.3(31) | – | 1.19(27) | – | 0.84(19) | – | 4, –, –, – |
| J1741+1351 | −8.93(8) | – | −7.43(17) | – | 11.62(13) | 11.71(1) | <1.2 | 0.93(4) | >0.83 | 1.08(5) | −, –, 10, 10 |
| J1811−2405 | 0.65(14) | 0.53(13) | −9.1(52) | – | 9.2(51) | – | <0.4 | – | >2.50 | – | 11, –, –, – |
| J1823−3021A | 0.31(24) | – | −8.2(17) | – | 8.2(17) | – | <7.0 | – | >0.14 | – | −, –, –, – |
| J2017+0603 | 2.35(8) | – | 0.17(16) | – | 2.35(8) | – | 1.2(5) | – | 0.9(4) | – | −, –, –, – |
| J2043+1711 | −6.12(27) | −7(2) | −11.2(5) | −11(2) | 12.8(4) | 13(2) | <4.4 | – | >0.23 | – | 12, 12, 12, – |
| J2214+3000 | 20.90(11) | – | −1.55(15) | – | 20.96(11) | – | 1.7(9) | – | 0.60(31) | – | −, –, –, – |
| J2302+4442 | −0.05(13) | – | −5.85(12) | – | 5.85(12) | – | <2.5 | – | >0.40 | – | −, –, –, – |
Notes. Quoted uncertainties on the measured parameters PMRA, PMDEC, and PX, are the 1 σ statistical error bars from Tempo2. In the cases where the parallax was not measurable, we quote 2σ upper limits based on the radio timing data. For pulsars with previously reported proper motion or parallax values, we report these results and give the associated references.
Reference. (1) – Hobbs et al. (2005); (2) – Burgay et al. (2006); (3) – Nice et al. (2005); (4) – Verbiest et al. (2009); (5) – Hotan et al. (2006); (6) – Ransom et al. (2011); (7) – Toscano et al. (1999); (8) – Bhalerao & Kulkarni (2011); (9) – Demorest et al. (2010); (10) – Espinoza et al. (2013); (11) – Ng et al. (2014); (12) – Guillemot et al. (2012).
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