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Table 4

Same as in Table 3, but for DR2new.

Pulsar Favoured models Red noise DM noise Time span


Ncoef A γ Ncoef A γ yr
J0030+0451 RN 10 X X X 9.78
J0613−0200 DM X X X 11 10.07
J0751+1807 DM X X X 92 10.08
J0900−3144 RN+DM 99 100 9.86
J1012+5307 RN+DM 92 16 10.08
J1022+1001 RN+DM 30 100 10.08
J1024−0719 DM X X X 15 10.08
J1455−3330 RN 80 X X X 9.27
J1600−3053 DM+SV X X X 97 9.91
J1640+2224 DM X X X 47 10.22
J1713+0747 RN+DM 10 73 10.08
J1730−2304 DM X X X 11 9.93
J1738+0333 DM X X X 24 9.98
J1744−1134 DM X X X 87 9.75
J1751−2857 DM X X X 25 9.43
J1801−1417 DM X X X 11 9.74
J1804−2717 DM X X X 23 9.54
J1843−1113 DM X X X 95 10.08
J1857+0943 DM X X X 20 9.98
J1909−3744 RN+DM 14 95 9.04
J1910+1256 DM X X X 20 9.91
J1911+1347 DM X X X 15 9.92
J1918−0642 DM X X X 75 10.08
J2124−3358 DM X X X 24 9.68
J2322+2057 NONE X X X X X X 9.68

Notes. Pulsars for which the preferred noise models have changed from Table 3 are highlighted.

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