Table 2.
Astrometric and spin properties of the 19 pulsars constituting our spider pulsar sample.
| Pulsar | Discovery article | Gal. lon. | Gal. lat. | P | DM | d |
|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (ms) | (pc cm−3) | (kpc) | ||
| J0023+0923 | Bangale et al. (2024) | 111.38 | −52.85 | 3.05 | 14.3 | 1.24 |
| J0610−2100 | Burgay et al. (2006) | 227.75 | −18.18 | 3.86 | 60.7 | 3.26 |
| J0636+5128 | Stovall et al. (2014) | 163.91 | 18.64 | 2.87 | 11.1 | 0.21 |
| J1124−3653 | Bangale et al. (2024) | 284.09 | 22.76 | 2.41 | 44.9 | 0.99 |
| J1513−2550 | Sanpa-Arsa (2016) | 338.82 | 26.96 | 2.12 | 46.9 | 3.96 |
| J1544+4937 | Bhattacharyya et al. (2013) | 79.17 | 50.17 | 2.16 | 23.2 | 2.98 |
| J1555−2908 | Ray et al. (2022) | 344.48 | 18.50 | 1.79 | 75.9 | 7.55 |
| J1628−3205 | Ray et al. (2012) | 347.43 | 11.48 | 3.21 | 42.1 | 1.22 |
| J1705−1903 | Morello et al. (2018) | 3.25 | 13.03 | 2.48 | 57.5 | 2.34 |
| J1719−1438 | Bailes et al. (2011) | 8.86 | 12.84 | 5.79 | 36.8 | 0.34 |
| J1731−1847 | Keith et al. (2010) | 6.89 | 8.15 | 2.35 | 106.5 | 4.77 |
| J1745+1017 | Barr et al. (2013) | 34.87 | 19.25 | 2.65 | 24.0 | 1.22 |
| J1959+2048 | Fruchter et al. (1988) | 59.20 | −4.70 | 1.61 | 29.1 | 1.73 |
| J2051−0827 | Stappers et al. (1996) | 39.19 | −30.41 | 4.51 | 20.7 | 1.47 |
| J2055+3829 | Guillemot et al. (2019) | 80.62 | −4.26 | 2.09 | 91.8 | 4.59 |
| J2115+5448 | Sanpa-Arsa (2016) | 95.04 | 4.11 | 2.60 | 77.4 | 3.11 |
| J2214+3000 | Ransom et al. (2011) | 86.86 | −21.67 | 3.12 | 22.6 | 1.68 |
| J2234+0944 | Ray et al. (2012) | 76.28 | −40.44 | 3.63 | 17.8 | 1.58 |
| J2256−1024 | Crowter et al. (2020) | 59.23 | −58.29 | 2.30 | 13.8 | 1.33 |
Notes. For each pulsar we list the discovery article, the galactic coordinates, the spin period P, the dispersion measure DM, and the distance d. The latter distance values are based on the DMs and were estimated using the YMW16 model for the distribution of free electrons in the Galaxy (Yao et al. 2017).
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