Table 1.
Properties of the ordinary and millisecond pulsars investigated with XMM-Newton in this study.
| Pulsar | ObsID | tPN | tM1 | tM2 | bPN | bM1 | bM2 | P | D1 | D2 | log Ė | NH, 21 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (ks) | (ks) | (ks) | (c/s) | (c/s) | (c/s) | (ms) | (kpc) | (kpc) | (ergs s−1) | |||
| J0711–6830 | 0823030601 | 11.9 (6.1) | 13.8 (9.8) | 13.8 (9.2) | 2.5 (TN) | 0.35 (M) | 0.35 (M) | 5 | 0.11 | 0.86 | 33.6 | 0.6 |
| J0745–5353 | 0823031401 | 18.9 (13.5) | 20.8 (18.4) | 20.8 (16.1) | 0.4 (TN) | 0.2 (TN) | 0.2 (TN) | 215 | 0.57 | 0.25 | 34.0 | 3.8 |
| J0942–5552 | 0823031301 | 18.7 (13.5) | 20.6 (20.2) | 20.6 (20.2) | 0.5 (TN) | 0.35 (TN) | 0.35 (TN) | 664 | 0.30 | 3.8 | 33.5 | 5.6 |
| J0945–4833 | 0823031101 | 17.7 (11.2) | 19.6 (17.5) | 19.6 (17.2) | 0.5 (TN) | 0.2 (TN) | 0.25 (TN) | 331 | 0.35 | 1.51 | 33.7 | 3.0 |
| J0954–5430 | 0823030401 | 14.7 (4.7) | 16.6 (6.9) | 16.6 (6.0) | 2.0 (M) | 0.35 (M) | 0.35 (M) | 473 | 0.43 | 3.96 | 34.2 | 6.2 |
| J0957–5432 | 0823031001 | 15.7 (5.6) | 17.6 (17.2) | 17.6 (17.3) | 0.8 (M) | 0.35 (M) | 0.35 (M) | 203 | 0.45 | 4.33 | 34.0 | 7.0 |
| J1000–5149 | 0823030301 | 7.0 (5.8) | 8.9 (6.2) | 8.9 (8.7) | 0.4 (TN) | 0.35 (M) | 0.35 (M) | 255 | 0.13 | 1.93 | 33.4 | 2.2 |
| J1003–4747 | 0823030201 | 14.7 (9.3) | 16.6 (16.4) | 16.6 (16.3) | 1.0 (TN) | 0.35 (M) | 0.35 (M) | 307 | 0.37 | 2.94 | 34.5 | 3.0 |
| J1017–7156 (B) | 0823030701 | 10 (5.3) | 11.9 (10.7) | 11.9 (10.0) | 0.6 (TN) | 0.2 (M) | 0.25 (M) | 2 | 0.26 | 2.98 | 33.8 | 2.9 |
| J1125–5825 (B) | 0823031601 | 18.7 (5.7) | 20.6 (16.9) | 20.6 (16.9) | 0.7 (TN) | 0.35 (M) | 0.35 (M) | 3 | 1.74 | 2.62 | 34.9 | 3.9 |
| J1543–5149 (B) | 0823030901 | 6.5 (5.3) | 8.4 (8.3) | 8.4 (8.2) | 0.4 (TN) | 0.35 (TN) | 0.35 (TN) | 2 | 1.15 | 2.42 | 34.9 | 1.6 |
| J1725–0732 | 0823031501 | 15.1 (12.3) | 17.0 (16.7) | 17.0 (16.7) | 0.4 (TN) | 0.35 (M) | 0.35 (M) | 240 | 0.20 | 1.90 | 33.1 | 1.8 |
| J1740–3015 | 0823030101 | 4.7 (1.7) | 6.6 (6.0) | 6.6 (5.7) | 1.0 (TN) | 0.35 (M) | 0.35 (M) | 607 | 0.40 | 2.94 | 34.9 | 4.7 |
| J1755–0903 | 0823030501 | 4.7 (3.9) | 6.6 (6.5) | 6.6 (6.5) | 0.4 (TN) | 0.35 (M) | 0.35 (M) | 191 | 0.23 | 1.79 | 33.6 | 2.0 |
Notes. Pulsar names and their XMM-Newton obsid’s are given in the first and second column. The pulsars in binary systems are marked with (B). The following six column displays EPIC-pn and EPIC-MOS total and GTI-filtered exposure times (given in parentheses) and the GTI filter for the background light curve and the corresponding filters for each EPIC detector. “TN” is thin filter and “M” is medium filter. Source properties are noted in the last five columns. P is the spin period in seconds, D1 is the best estimate of the pulsar distance in kpc according to ATNF pulsar catalog which uses the YMW+17 DM-based distance as default, D2 is the distance in kpc based on the NE2001 model, log Ė is the common logarithm of the spin-down energy loss rate in ergs s−1 and NH is the hydrogen column density in unit of 1021 cm−2 estimated from the DM as outlined in Sect. 2.4.
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