Table 3
Observational properties of the ATNF pulsars with newly discovered X-ray counterparts in eRASS:4 data.
| PSR | γ−ray counterpart | P s | Ṗ s s−1 | d kpc | Age yr |  erg s−1 |
Rate ct s−1 | ℒdet |
|---|---|---|---|---|---|---|---|---|
| J0837−2454 | 0.62941 | 3.49 × 10−13 | 0.20 | 2.86 × 104 | 5.50 × 1034 | 0.0125 | 61.6 | |
| J0711−6830 | 0.00549 | 1 . 49 × 10−20 | 0.11 | 5.84 × 109 | 3.61 × 1033 | 0.0056 | 16.2 | |
| J1902−5105 | 4FGL J1902.0−5105 | 0.00174 | 9.20 × 10−21 | 1.65 | 3.00 × 109 | 6.87 × 1034 | 0.0194 | 5.3 |
| J1045−4509 | 0.00747 | 1.76 × 10−20 | 0.34 | 6.70 × 109 | 1.70 × 1033 | 0.0129 | 7.4 | |
| J1125−6014 | 4FGL J1126.4−6011 | 0.00263 | 3.73 × 10−21 | 0.99 | 1.12 × 1010 | 8.09 × 1033 | 0.0151 | 11.1 |
| J1312+0051 | 4FGL J1312.7+0050 | 0.00423 | 1.75 × 10−20 | 1.47 | 3.82 × 109 | 9.15 × 1033 | 0.0406 | 31.6 |
| J0509+0856 | 0.00406 | 4.41 × 10−21 | 0.82 | 1 .46 × 1010 | 2.61 × 1033 | 0.0150 | 7.4 | |
| J0514−4408 | 4FGL J0514.6−4408 | 0.32027 | 2.04 × 10−15 | 0.97 | 2.48 × 106 | 2.45 × 1033 | 0.0134 | 17.3 |
| J1207−5050 | 4FGL J1207.4−5050 | 0.00484 | 6.06 × 10−21 | 1.27 | 1.27 × 1010 | 2.11 × 1033 | 0.0174 | 14.1 |
| J0952−0607 | 4FGL J0952.1−0607 | 0.00141 | 4.77 × 10−21 | 7.60 | 4.69 × 109 | 6.67 × 1034 | 0.0325 | 12.3 |
| J0610−2100 | 4FGL J0610.2−2100 | 0.00386 | 1.23 × 10−20 | 3.26 | 4.96 × 109 | 8.45 × 1033 | 0.0241 | 15.6 |
| J1439−5501 | 4FGL J1440.2−5505 | 0.02864 | 1.42 × 10−19 | 0.66 | 3.20 × 109 | 2.38 × 1032 | 0.0180 | 13.3 |
| B1036−45 | 0.66199 | 1.25 × 10−15 | 0.92 | 8.38 × 106 | 1.71 × 1032 | 0.0167 | 11.6 | |
| J1405−5641 | 0.61757 | 1.20 × 10−15 | 12.38 | 8.17 × 106 | 2.01 × 1032 | 0.0133 | 6.6 | |
| J1057−5851 | 4FGL J1056.9−5852 | 0.62037 | 1.01 × 10−13 | 9.77 × 104 | 1.66 × 1034 | 0.0099 | 8.4 |
Notes. The individual columns are as follows: PSR: Pulsar name, γ-ray counterpart: Name of the source in the 4FGL catalog. The pulsar parameters P (rotation period), Ṗ (period derivative), d (distance), (spin−down) age, and 
(spin-down power) are taken from the ATNF pulsar database (Manchester et al. 2005). Rate is the count rate in the 0.2–2.3 ke V band. ℒdet is the detection likelihood for the 0.2–2.3 keV band (Brunner et al. 2022). The list is sorted in descending order of 
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