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Table 1

Summary of observations.

Source name P DM β Span Nglow Ncore med(σToA) med(σDM) med Nchan PTA
(J2000) (ms) (deg) (yr) (μs)
J0030+0451 4.9 4.3 1.4 7.0 355 79 7 16 1.0 10 E N
J0034−0534 1.9 13.8 -8.5 7.0 1041 78 1 3 1.0 20 E
J0218+4232 2.3 61.2 27.0 6.5 539 74 13 35 0.9 10 E
J0407+1607 25.7 35.6 -4.7 6.4 386 65 24 56 1.0 10
J0621+1002 28.9 36.5 -13.3 7.0 10 74 251 568 1.3 10 (*) E
J0645+5158 8.9 18.2 28.9 6.9 268 4 3 7 0.9 10 N
J0740+6620 2.9 15.0 44.1 4.8 261 0 2 4 0.9 10 N
J0751+1807 3.5 30.2 -2.8 7.1 0 71 34 89 0.6 10 (*) E
J0952−0607 1.4 22.4 -17.9 2.9 37 33 9 14 1.0 8 (*)
J1012+5307 5.3 9.0 38.8 7.1 1210 79 4 12 1.2 10 E N
J1022+1001 16.5 10.3 -0.1 7.1 1224 80 5 12 1.2 20 E P N
J1024−0719 5.2 6.5 -16.0 7.1 5 81 32 80 0.9 8 (*) E P N
J1125+7819 4.2 11.2 62.5 4.8 282 0 3 8 0.9 10 N
J1300+1240 (a) 6.2 10.2 17.6 7.1 377 80 3 7 0.8 20 -
J1400−1431 3.1 4.9 -2.2 4.3 145 49 7 6 0.8 8 (*)
J1544+4937 2.2 23.2 65.9 5.6 5 53 19 59 1.0 6 (*)
J1552+5437 2.4 22.9 70.7 3.7 0 41 3 7 0.9 10 (*)
J1640+2224 3.2 18.4 44.1 7.1 435 79 7 18 0.8 8 E N
J1658+3630 33.0 3.0 58.7 2.6 164 6 7 18 0.9 10
J1713+0747 4.6 16.0 30.7 7.0 7 79 12 29 0.6 10 (*) E P N
J1730−2304 8.1 9.6 0.2 6.5 0 74 21 49 0.8 10 (*) E P
J1738+0333 5.9 33.8 26.9 7.1 0 77 39 110 0.7 6 (*) E N
J1744−1134 4.1 3.1 11.8 7.0 372 79 14 19 0.9 10 E P N
J1853+1303 4.1 30.6 35.7 6.5 1 72 21 50 0.8 8 (*) E N
J1857+0943 (b) 5.4 13.3 32.3 7.1 0 75 41 82 1.3 10 (*) E P N
J1911−1114 3.6 31.0 11.1 7.0 0 74 32 68 0.9 10 E
J1918−0642 7.6 26.6 15.4 7.0 0 75 55 136 0.8 10 (*) E N
J1923+2515 3.8 18.9 46.7 6.6 0 73 6 15 0.9 10 (*) N
J1944+0907 5.2 24.4 29.9 6.5 35 64 33 80 0.8 6 (*) N
J1955+2908 (c) 6.1 104.5 48.7 6.6 0 74 100 273 0.9 10 (*) E N
J2043+1711 2.4 20.7 34.0 6.7 3 71 6 17 0.9 10 (*) N
J2051−0827 4.5 20.7 8.8 6.5 6 74 14 29 0.7 10 (*)
J2145−0750 16.1 9.0 5.3 7.0 1010 81 3 9 1.1 20 E P N
J2222−0137 32.8 3.3 8.0 3.8 130 41 22 49 0.9 10 (*)
J2302+4442 5.2 13.7 45.7 6.2 0 71 20 51 0.8 10 (*) N
J2317+1439 3.4 21.9 17.7 7.0 381 77 2 6 1.0 10 E N

Notes. Given are the pulsar name in J2000 coordinates, the pulse period P, the catalogue DM, the ecliptic latitude β, the total time span of the observations, the number of observations with GLOW and the LOFAR Core Nglow and Ncore, the median frequency-integrated ToA uncertainty, the median uncertainty of individual DM measurements, the median reduced χ2 of the individual DM fits, and the number of frequency channels in each observation. The last column shows whether the pulsar is used in different PTA projects (i.e. E: European Pulsar Timing Array, EPTA; P: Parkes Pulsar Timing Array, PPTA; N: North American Nanohertz Observatory for Gravitational Waves, NANOGrav; see Verbiest et al. 2016; Arzoumanian et al. 2018). A pulsar observed by any of the PTAs is also used by the International Pulsar Timing Array (IPTA). (*) For these pulsars, an analytic standard template without frequency resolution was used. (a) PSR B1257+12 (b) PSR B1855+09 (c) PSR B1953+29.

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