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Table 1.

J1513 and J2017 parameters obtained from Sanpa-arsa (2016), the ATNF catalogue, and the Third Fermi Large Area Telescope catalogue of γ-ray pulsars (Smith et al. 2023).

MSP J2017 J1513
RA α (J2000) 20h17m46.​​s1478(8) 15h13m23.​​s32059(6)
Dec δ (J2000) −16 ° 14′15.​​″51(5) −25 ° 50′31.​​″285(3)
Galactic longitude l, deg 27.314 338.820
Galactic latitude b, deg −26.220 26.964
Spin period P, ms 2.3142872649224(4) 2.1190675651177(1)
Period derivative P ˙ $ \dot{P} $, s s−1 2.45(5) × 10−21 21.61(2) × 10−21
Orbital period Pb, d 0.0978252578(4) 0.1786354505(8)
Projected semi-major axis x, lt-s 0.043655(5) 0.0408132(7)
Epoch of ascending node Tasc, MJD 56704.756314(2) 56728.4539340(6)
Mass function fM, M 9.334(3) × 10−6 2.2874(1) × 10−6
Dispersion measure DM, pc cm−3 25.4380(4) 46.86(7)
Distance DYMW16, kpc 1.4 4.0
Distance DNE2001, kpc 1.1 2.0
Characteristic age τ c P / 2 P ˙ $ \tau_c\equiv P/2\dot{P} $, Gyr 15 1.55
Spin-down luminosity E ˙ $ \dot{E} $, erg s−1 7.8 × 1033 9.0 × 1034
Minimum companion mass Mc,  min, M 0.03 0.02

p.m. in RA direction μαcos δ, mas yr−1 −6.3(1)
p.m. in Dec direction μδ, mas yr−1 −3.5(4)

Notes. Numbers in parentheses denote 1σ uncertainties relating to the last significant digit.

DYMW16 and DNE2001 are dispersion measure distances derived using the YMW16 (Yao et al. 2017) and NE2001 (Cordes & Lazio 2002) models for the distribution of free electrons in the Galaxy, respectively. The minimum companion mass was calculated for the pulsar mass of Mp = 1.4 M and orbital inclination of i = 90°. p.m. = proper motion.

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