Timing irregularities and glitches from the pulsar monitoring campaign at IAR

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Table 1.

Observations analysed in this work.

Pulsar	# of observations			Data span	⟨t_obs⟩	⟨S/N⟩	⟨σ_TOA⟩	P	Ṗ	Age	Previous glitches

	A1	A2	Total	(MJD)	(min)		(μs)	(s)	(10⁻¹⁴ s s⁻¹)	(kyr)
J0742−2822	345	408	753	58832–60149	27	6.6	190	0.167	1.68	157	9
J0835−4510	312	579	891	59264–60278	216	1024	7.1	0.089	12.5	11	22
J1048−5832	241	171	412	59031–60294	96	5.7	181	0.123	9.61	20	9
J1644−4559	229	403	632	58979–60294	35	7.3	35	0.455	2.01	359	4
J1731−4744	217	23	240	58751–60294	96	4.6	303	0.830	16.3	80	6
J1740−3015	0	316	316	59330–60314	114	8.4	286	0.606	46.6	20	38

Notes. ⟨t_obs⟩ is the typical observing time for each pulsar, and ⟨S/N⟩ and ⟨σ_TOA⟩ are their typical S/N and TOA uncertainty, respectively. The number of previous glitches was extracted from Basu et al. (2022).

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