Improving pulsar timing precision through superior time-of-arrival creation

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Table 3

Overview of the pulsars’ properties.

PSR	P (ms)	$\dot{P}$ $\dot P$ (10⁻²⁰)	P_b (days)	DM (cm⁻³ pc)	S_1.4 (mJy)	Ref.
J0030+0451	4.865	1.02	−	4.33	0.6	Lommen et al. (2000); Verbiest et al. (2016)
J0613−0200	3.062	0.96	1.20	38.79	1.7	Lorimer et al. (1995); Verbiest et al. (2016)
J1012+5307	5.26	1.71	0.60	9.02	2.8	Nicastro et al. (1995); Lange et al. (2001)
J1022+1001	16.453	4.33	7.81	10.25	6.1	Camilo et al. (1996); Desvignes et al. (2016)
J1024−0719	5.162	1.86	−	6.49	1.5	Bailes et al. (1997); Manchester et al. (2013)
J1600−3053	3.598	0.95	14.35	52.33	2.5	Jacoby et al. (2007); Ord et al. (2006); Manchester et al. (2013)
J1640+2224	3.163	0.28	175.46	18.43	0.4	Foster et al. (1995); Desvignes et al. (2016)
J1744−1134	4.075	0.86	−	3.14	1.0	Bailes et al. (1997)
J1857+0943	5.362	1.78	12.33	13.30	3.3	Segelstein et al. (1986); Verbiest et al. (2016)
J1909−3744	2.95	1.40	1.53	10.39	1.0	Jacoby et al. (2003); Desvignes et al. (2016)
J1918−0642	7.646	2.57	10.91	26.55	0.6	Edwards & Bailes (2001b); Janssen et al. (2010)
J2010−1323	5.223	0.48	−	22.16	1.6	Jacoby et al. (2007)
J2317+1439	3.445	0.24	2.46	21.90	4.0	Camilo et al. (1993); Verbiest et al. (2016)

Notes. The pulsar’s rotation period (P), spin-down ( $\dot{P}$ $\dot P$ ), orbital period (P_b), DM, and flux density at 1.4 GHz (S _1.4) are given.

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