Table 1.
Pulsar properties used for the injection.
| Pulsar | Tobs [yr] | RMSToAs [μs] | Noise model | log10ARN | γRN | nRN | log10ADM | γDM | nDM |
|---|---|---|---|---|---|---|---|---|---|
| J0030+0451 | 22 | 2.47 | RN | −15.18 | 5.71 | 10 | – | – | – |
| J0613-0200 | 22.9 | 3.4 | RN + DM | −14.87 | 5.05 | 10 | −13.51 | 2.13 | 144 |
| J0751+1807 | 24.2 | 2.11 | DM | – | – | – | −13.52 | 3.17 | 60 |
| J0900-3144 | 13.6 | 3.08 | RN + DM | −12.76 | 1.09 | 138 | −13.48 | 3.43 | 151 |
| J1012+5307 | 23.7 | 1.43 | RN + DM | −13.05 | 1.2 | 149 | −13.6 | 1.62 | 45 |
| J1022+1001 | 24.5 | 1.16 | RN + DM | −13.77 | 3.05 | 30 | −13.22 | 0.02 | 100 |
| J1024-0719 | 23.1 | 1.41 | DM | – | – | – | −13.48 | 2.31 | 34 |
| J1455-3330 | 15.7 | 2.74 | RN | −13.18 | 1.67 | 49 | – | – | – |
| J1600-3053 | 14.3 | 2.18 | DM | – | – | – | −13.82 | 3.89 | 26 |
| J1640+2224 | 24.4 | 1.27 | DM | – | – | – | −13.44 | 0.41 | 146 |
| J1713+0747 | 24.5 | 1.04 | RN + DM | −13.95 | 2.76 | 11 | −13.5 | 1.63 | 148 |
| J1730-2304 | 16.1 | 1.34 | DM | – | – | – | −13.27 | 2.49 | 10 |
| J1738+0333 | 14.1 | 3.2 | RN | −12.93 | 1.89 | 11 | – | – | – |
| J1744-1134 | 24 | 1.25 | RN + DM | −16.16 | 6.44 | 9 | −13.41 | 0.93 | 151 |
| J1751-2857 | 14.7 | 3.44 | DM | – | – | – | −12.76 | 2.3 | 41 |
| J1801-1417 | 13.7 | 4.88 | DM | – | – | – | −12.3 | 1.33 | 14 |
| J1804-2717 | 14.7 | 2.85 | DM | – | – | – | −12.8 | 0.66 | 38 |
| J1843-1113 | 16.8 | 4.18 | DM | – | – | – | −12.67 | 1.98 | 73 |
| J1857+0943 | 24.1 | 2.44 | DM | – | – | – | −13.41 | 2.7 | 10 |
| J1909-3744 | 15.7 | 1.17 | RN + DM | −15.14 | 5.13 | 20 | −13.61 | 1.45 | 151 |
| J1910+1256 | 15.2 | 3.32 | DM | – | – | – | −13.28 | 2.84 | 10 |
| J1911+1347 | 14.2 | 2.12 | DM | – | – | – | −13.64 | 3.18 | 10 |
| J1918-0642 | 19.7 | 2.32 | DM | – | – | – | −13.94 | 3.81 | 138 |
| J2124-3358 | 16 | 2.45 | DM | – | – | – | −13.07 | 1.03 | 41 |
| J2322+2057 | 14.7 | 4.44 | – | – | – | – | – | – | – |
Notes. For each pulsar in the array, the following properties are listed: name of the pulsar, observation time span, RMS of the timing residual, contributions to the noise model found through model selection in the single pulsar noise analysis of EPTA DR2full and the maximum likelihood values of the slope, the amplitude and the number of Fourier bins of RN and DM as obtained from the noise analysis of EPTA DR2full (EPTA Collaboration et al. 2023b). These values are used in the noise injection.
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