Table 3
Summary of the timing parallax measurements in the EPTA DR2.
| Pulsar name | ϖmes (mas) | S1400 (mJy) | Dcorr (kpc) | ϖref (mas) | Reference | µ (mas yr−1) | Vtrans (km s−1) |
|---|---|---|---|---|---|---|---|
| J0030+0451 | 3.09 ± 0.06 | 1.09 |  |
 |
Ding et al. (2023) |  |
 |
| J0613−0200 | 1.00 ± 0.05 | 2.25 |  |
 |
DR1 |  |
 |
| J0751+1807 | 0.85 ± 0.04 | 1.35 |  |
 |
DR1 |  |
 |
| J1012+5307 | 0.90 ± 0.08 | 3.8 |  |
 |
Ding et al. (2023) |  |
 |
| J1022+1001 | 1.16 ± 0.08 | 3.9 |  |
 |
Deller et al. (2019) |  |
 |
| J1024−0719 | 1.01 ± 0.04 | 1.5 |  |
 |
Ding et al. (2023) |  |
 |
| J1455−3330 | 1.3 ± 0.1 | 0.73 |  |
 |
DR1 |  |
 |
| J1600−3053 | 0.72 ± 0.02 | 2.44 |  |
 |
Reardon et al. (2021) |  |
 |
| J1640+2224 | 0.8 ± 0.2 | 0.46 |  |
 |
Ding et al. (2023) |  |
 |
| J1713+0747 | 0.88 ± 0.01 | 8.3 |  |
 |
DR1 |  |
 |
| J1730−2304 | 2.08 ± 0.06 | 4.0 |  |
 |
Ding et al. (2023) |  |
 |
| J1738+0333 | – | 0.34 | – |  |
Freire et al. (2012) |  |
 |
| J1744−1134 | 2.58 ± 0.03 | 2.6 |  |
 |
DR1 |  |
 |
| J1751−2857 | 1.1 ± 0.4 | 0.46 |  |
– | – |  |
 |
| J1801−1417 | 0.8 ± 0.3 | 1.54 |  |
– | – |  |
 |
| J1804−2717 | 1.1 ± 0.3 | 0.4 |  |
– | – |  |
 |
| J1857+0943 | 0.89 ± 0.06 | 5.0 |  |
 |
DR1 |  |
 |
| J1909−3744 | 0.94 ± 0.02 | 1.8 |  |
 |
Liu et al. (2020) |  |
 |
| J1911+1347 | 0.40 ± 0.09 | 0.9 |  |
– | – |  |
 |
| J1918−0642 | 0.75 ± 0.07 | 0.58 |  |
 |
Ding et al. (2023) |  |
 |
| J2124−3358 | 2.1 ± 0.1 | 4.5 |  |
 |
DR1 |  |
 |
Notes. The ϖmes column gives the median and 68.3 percentiles of the marginalised posteriod distribution. S1400 gives the pulsar flux densities that were used to infer the bias-corrected distances, Dcorr (all taken from the ATNF catalogue v1.69 (Hobbs et al. 2004); see Sect. 5.1 for details on parallax inversion). The last two columns list the magnitude of the proper motion and the inferred transverse velocity (Vtrans = 4.74µDcorr) of the system, respectively.
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