Table 3.
The properties of 2MASS J02105640+584517.
| d | Mc | Teff | Ref. |
|---|---|---|---|
| (kpc) | (M⊙) | (K) | |
| 2.5(5)( * ) | – | – | Cordes & Lazio (2002) |
| 2.0(4)( * ) | – | – | Yao et al. (2017) |
 |
 |
 |
Anders et al. (2019) |
| – | – | 7840(253) | Xiang et al. (2019) |
 |
 |
 |
Queiroz et al. (2020) |
 |
– | – | Bailer-Jones et al. (2021) |
 |
 |
 |
Anders et al. (2022) |
 |
 |
 |
Gaia Collaboration (2023) |
| – | – | 14 279(603) | Xiang et al. (2022) |
| – | 3.5–3.8 | 14 275(133) | This paper |
Notes. Shown are the distance, d, mass, Mc, and effective temperature, Teff as documented in different catalogues. The uncertainties are 68% confidence intervals as upper and lower bounds or 1σ uncertainties in parentheses. Distances denoted with ( * )are derived from the location and DM of the pulsar using the NE2001 (Cordes & Lazio 2002) and YMW16 (Yao et al. 2017) Galactic electron density models.
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