Table 3
Properties of the MSPs used to test the polarization calibration procedure described in Sect. 3.
| Pulsar name (Julian) | Pulsar name (Besselian) | Discovery article | P (ms) | DM (pc cm−3) | Nobs | Min. epoch (MJD) | Max. epoch (MJD) | R1 | R2 |
|---|---|---|---|---|---|---|---|---|---|
| J0125-2327 | Morello et al. (2019) | 3.675 | 9.60 | 1126 | 57928.3 | 60485.3 | 1.029 | 1.000 | |
| J0613-0200 | Lorimer et al. (1995) | 3.062 | 38.78 | 409 | 55817.3 | 60484.5 | 0.996 | 1.009 | |
| J1022+1001 | Camilo et al. (1996) | 16.453 | 10.26 | 449 | 55839.4 | 60482.7 | 0.971 | 1.026 | |
| J1024-0719 | Bailes et al. (1997) | 5.162 | 6.49 | 583 | 55819.5 | 60481.7 | 1.138 | 0.868 | |
| J1600-3053 | Jacoby et al. (2007) | 3.598 | 52.32 | 716 | 55800.7 | 60483.9 | 1.019 | 0.993 | |
| J1643-1224 | Lorimer et al. (1995) | 4.622 | 62.40 | 312 | 55836.6 | 60483.9 | 1.010 | 0.979 | |
| J1730-2304 | Lorimer et al. (1995) | 8.123 | 9.62 | 356 | 55923.5 | 60485.0 | 1.035 | 0.962 | |
| J1744-1134 | Bailes et al. (1997) | 4.075 | 3.14 | 342 | 55805.8 | 60476.0 | 1.130 | 0.886 | |
| J1857+0943 | B1855+09 | Segelstein et al. (1986) | 5.362 | 13.30 | 233 | 55800.8 | 60484.0 | 1.014 | 0.968 |
| J1909-3744 | Jacoby et al. (2003) | 2.947 | 10.39 | 702 | 55812.8 | 60473.1 | 1.050 | 0.952 | |
| J2124-3358 | Bailes et al. (1997) | 4.931 | 4.60 | 525 | 55805.9 | 60475.2 | 0.995 | 0.994 | |
| J2145-0750 | Bailes et al. (1994) | 16.052 | 9.00 | 554 | 55804.0 | 60483.1 | 1.010 | 0.992 |
Notes. For each MSP we list the rotational period, dispersion measure, the number of 1.4 GHz NUPPI observations considered in the analysis, and corresponding minimum and maximum epochs. The last two columns respectively give the median S/N and TOA uncertainty ratios, between corrected and uncorrected data (see Sect. 4.1 for details).
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