Table 4.
Properties of ordinary and ms-pulsars with possible counterparts in the 4XMM-DR10 catalog for which we could not find a respective note in the literature or that were previously marked as upper limits.
| Pulsar | ObsID | ΔX − R | θ | IAU name | ML | PN 0.3 − 2 keV |
MOS1 0.3 − 2 keV |
MOS2 0.3 − 2 keV |
|||
|---|---|---|---|---|---|---|---|---|---|---|---|
| (arcsec) | (arcmin) | Ns | S | Ns | S | Ns | S | ||||
| (counts) | (σ) | (counts) | (σ) | (counts) | (σ) | ||||||
| J0340+4130 | 0605470101 | 4.74 | 7.8 | 4XMM J034023.3+413040 | 12.0 | 11.4 ± 5.4 | 2.1 | 13.9 ± 5.6 | 2.5 | 13.6 ± 4.3 | 3.1 |
| J1435−5954 | 0692050101 | 2.59 | 16.9 | 4XMM J143500.1–595452 | 11.3 | 66.8 ± 17.9 | 3.7 | − | − | − | − |
| J1622−0315 | 0784770401 | 0.84 | 1.7 | 4XMM J162259.6–031538 | 63.5 | 33.9 ± 7.8 | 4.3 | 24.1 ± 6.8 | 3.5 | 20.1 ± 6.9 | 2.9 |
| J1535−4114 | 0652610201 | 5.6 | 4.3 | 4XMM J153516.5–411402 | 12.7 | 72.5 ± 16.5 | 4.4 | 21.0 ± 9.8 | 2.1 | 19.8 ± 8.5 | 2.3 |
| J1643−1224 | 0742520101 | 1.5 | 1.1 | 4XMM J164338.0–122458 | 112.7 | 66.8 ± 11.3 | 5.9 | 24.4 ± 6.4 | 3.8 | 22.3 ± 6.3 | 3.5 |
| J1831−0952 | 0822330101 | 2.2 | 2.3 | 4XMM J183134.1–095201 | 96.9 | − | − | 28.9 ± 9.6 | 3.0 | 29.0 ± 9.7 | 3.0 |
| J1857+0943 | 0742520201 | 1.3 | 1.2 | 4XMM J185736.4+094317 | 38.3 | 27.9 ± 6.8 | 4.1 | 7.1 ± 4.5 | 1.6 | 13.8 ± 4.7 | 2.9 |
| J1926−1314 | 0742620101 | 5.5 | 1.1 | 4XMM J192653.7–131358 | 6.9 | 59.6 ± 16.7 | 3.5 | 13.5 ± 8.2 | 1.6 | 27.6 ± 9.6 | 2.8 |
Notes. ΔX − R column displays angular separation in ″ between the pulsar’s radio timing position and the centroid of the nearest X-ray source according to 4XMM-DR10. θ is the EPIC-pn off-axis angle. ML is the reported 4XMM-DR10 maximum likelihood in the energy band 0.2–12.0 keV. Background-corrected counts Ns at the optimized X-ray source position and their corresponding significance are displayed for EPIC-pn and EPIC-MOS1/MOS2. PSR J1831–0952 has a ∼6σ significance in 0.3–4.5 keV with Epic-MOS cameras. The off-axis angle is given for Epic-MOS1.
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