Table 3
Favoured models listed for the 25 pulsars using both EPTA and InPTA data (for 10 common MSPs; DR2full+) along with estimated values for chromatic and achromatic noise models.
| Pulsar | PTA | Favoured | Red noise | DM noise | Time span | ||||
|---|---|---|---|---|---|---|---|---|---|
| models | Ncoef | A | γ | Ncoef | A | γ | yr | ||
| J0030+0451 | EPTA | RN | 10 |  |
 |
X | X | X | 21.96 |
| J0613-0200 | EPTA+InPTA | RN+DM | 10 |  |
 |
129 |  |
 |
23.83 |
| J0751+1807 | EPTA+InPTA | DM | X | X | X | 115 |  |
 |
25.12 |
| J0900-3144 | EPTA | RN+DM | 135 |  |
 |
150 |  |
 |
13.64 |
| J1012+5307 | EPTA+InPTA | RN+DM | 149 |  |
 |
47 |  |
 |
24.61 |
| J1022+1001 | EPTA+InPTA | RN+DM | 30 |  |
 |
100 |  |
 |
25.37 |
| J1024−0719 | EPTA | DM | X | X | X | 34 |  |
 |
23.14 |
| J1455−3330 | EPTA | RN | 49 |  |
 |
X | X | X | 15.72 |
| J1600−3053 | EPTA+InPTA | RN+DM | 21 |  |
 |
148 |  |
 |
15.42 |
| J1640+2224 | EPTA | DM | X | X | X | 145 |  |
 |
24.44 |
| J1713+0747 | EPTA+InPTA | RN+DM | 12 |  |
 |
148 |  |
 |
24.5 |
| J1730-2304 | EPTA | DM | X | X | X | 10 |  |
 |
16.1 |
| J1738+0333 | EPTA | RN | 11 |  |
 |
X | X | X | 14.12 |
| J1744−1134 | EPTA+InPTA | RN+DM | 10 |  |
 |
150 |  |
 |
25.14 |
| J1751-2857 | EPTA | DM | X | X | X | 41 |  |
 |
14.69 |
| J1801-1417 | EPTA | DM | X | X | X | 14 |  |
 |
13.71 |
| J1804-2717 | EPTA | DM | X | X | X | 38 |  |
 |
14.73 |
| J1843-1113 | EPTA | DM | X | X | X | 73 |  |
 |
16.8 |
| J1857+0943 | EPTA+InPTA | DM | X | X | X | 11 |  |
 |
25.11 |
| J1909-3744 | EPTA+InPTA | RN+DM | 20 |  |
 |
150 |  |
 |
17.14 |
| J1910+1256 | EPTA | DM | X | X | X | 10 |  |
 |
15.21 |
| J1911+1347 | EPTA | DM | X | X | X | 10 |  |
 |
14.2 |
| J1918−0642 | EPTA | DM | X | X | X | 138 |  |
 |
19.71 |
| J2124−3358 | EPTA+InPTA | DM | X | X | X | 18 |  |
 |
17.15 |
| J2322+2057 | EPTA | NONE | X | X | X | X | X | X | 14.68 |
Notes. The second column lists the PTAs that contributed to the dataset for each pulsar. The third column reports the favoured model. Columns 4 to 9 report the estimated number of coefficients, amplitude, and slope (medians with 95% confidence intervals) for the achromatic and chromatic noise processes, respectively. The last column reports the total time span for each of the pulsars.
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