Table 2.
Properties of the selected ordinary and millisecond pulsars investigated in this study.
| Pulsar | ObsID | ΔX − R | PN 0.3 − 2 keV |
MOS1 0.3 − 2 keV |
MOS2 0.3 − 2 keV |
Combined EPIC |
||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Ns | S | UL | Ns | S | UL | Ns | S | UL | Ns | S | ML | |||
| (arcsec) | (counts) | (σ) | (c/s) | (counts) | (σ) | (c/s) | (counts) | (σ) | (c/s) | (counts | (σ) | |||
| J0711–6830 | 0823030601 | 1.7 | 23.5 ± 13.0 | 1.8 | 0.0080 | − | − | 0.0005 | 11.3 ± 4.7 | 2.4 | 0.0018 | 54.8 ± 15.7 | 3.5 | 14.9 |
| J0745–5353 | 0823031401 | 1.5 | 27.2 ± 7.6 | 3.6 | − | 6.2 ± 4.0 | 1.6 | 0.0006 | 8.1 ± 4.3 | 1.9 | 0.0007 | 39.6 ± 9.2 | 4.3 | 16.2 |
| J0942–5552 | 0823031301 | 9.7 | 31.7 ± 10.3 | 3.1 | − | − | − | 0.0004 | − | − | 0.0006 | − | − | − |
| J0945–4833 | 0823031101 | 2.3 | 14.8 ± 7.2 | 2.2 | 0.0021 | 3.3 ± 5.1 | − | 0.0007 | − | − | 0.0004 | − | − | − |
| J0954–5430 | 0823030401 | 1.2 | 4.4 ± 4.2 | 1.1 | 0.0021 | 1.7 ± 3.2 | − | 0.0009 | 2.5 ± 2.9 | − | 0.0012 | − | − | − |
| J0957–5432 | 0823031001 | 8.5 | 9.0 ± 5.8 | 1.6 | 0.0024 | 8.3 ± 5.6 | 1.5 | 0.0008 | − | − | 0.0003 | − | − | − |
| J1000–5149 | 0823030301 | 2.7 | − | − | 0.0007 | − | − | 0.0005 | − | − | 0.0010 | − | − | − |
| J1003–4747 | 0823030201 | 2.1 | 10.5 ± 8.4 | 1.3 | 0.0019 | 3.4 ± 3.8 | − | 0.0005 | − | − | 0.0002 | − | − | − |
| J1017–7156 | 0823030701 | 5.3 | 1.6 ± 3.9 | − | 0.0015 | − | − | 0.0002 | − | − | 0.0003 | − | − | |
| J1125–5825 | 0823031601 | 0.6 | 18.8 ± 6.7 | 2.8 | 0.0038 | 17.4 ± 6.3 | 2.8 | 0.0012 | 10.3 ± 5.2 | 2.0 | 0.0009 | 47.4 ± 10.2 | 4.7 | 20.9 |
| J1543–5149 | 0823030901 | 1.2 | 4.0 ± 4.0 | 1.0 | 0.0018 | 3.8 ± 3.6 | 1.2 | 0.0011 | − | − | 0.0007 | − | − | − |
| J1725–0732 | 0823031501 | 4.4 | 3.3 ± 3.8 | − | 0.0006 | 1.6 ± 2.7 | − | 0.0004 | − | − | 0.0003 | − | − | − |
| J1740–3015 | 0823030101 | 7.8 | 6.4 ± 3.5 | 1.8 | 0.0064 | − | − | 0.0008 | − | − | 0.0008 | − | − | − |
| J1755–0903 | 0823030501 | 0.3 | 6.2 ± 4.1 | 1.5 | 0.0031 | − | − | 0.0006 | − | − | 0.0009 | − | − | − |
Notes. The ΔX − R column displays angular separation in arcseconds between the pulsar’s radio timing position and the centroid of the nearest X-ray source. Background-subtracted counts Ns at the optimized X-ray source position and their corresponding significance S according to Eq. (1) are listed for each detector, as well as the ML for the detections considering all EPIC instruments together. The 3σ upper limits (UL) for individual instruments are Bayesian upper limits according to Kraft et al. (1991). The ML values are given in 0.3–2.0 keV for PSRs J0745–5353 and J1125–5825 and in 0.3–4.5 keV for PSR J0711–6830.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.