Table 1.
Final source selection, encompassing 14 pulsars.
| Name | Time span | Observing | Galactic | Period | Ecliptic | DM | Log | Observations | ||
|---|---|---|---|---|---|---|---|---|---|---|
| sites | coo. [deg] | [ms] | latitude [deg] | [pc cm−3] | M(eDM) | per template | ||||
| J0030+0451 | 2013-01 | 2019-05 | 7 | 113.1 | −57.6 | 4.9 | 1.45 | 4.3 | −4.02 | 215 |
| J0034−0534 | 2012-12 | 2019-05 | 6 | 111.5 | −68.1 | 1.9 | −8.53 | 13.8 | −4.66 | 227 |
| J0051+0423 | 2013-08 | 2019-05 | 5 | 123. | −58.5 | 354.7 | −1.05 | 13.9 | −3.17 | 208 |
| J0304+1932 | 2013-08 | 2019-05 | 6 | 161.1 | −33.3 | 1387.6 | 2.10 | 15.7 | −3.0 | 208 |
| J0407+1607 | 2013-08 | 2019-05 | 7 | 176.6 | −25.7 | 25.7 | −4.74 | 35.6 | −3.37 | 216 |
| J0826+2637 | 2013-08 | 2019-05 | 7 | 197.0 | 31.7 | 530.7 | 7.24 | 19.5 | −3.79 | 150 |
| J1022+1001 | 2012-12 | 2019-08 | 8 | 231.8 | 51.1 | 16.5 | −0.06 | 10.3 | −3.95 | 290 |
| J1136+1551 | 2013-08 | 2019-05 | 6 | 241.9 | 69.2 | 1187.9 | 12.16 | 4.8 | −3.97 | 299 |
| J1300+1240 | 2012-12 | 2019-08 | 6 | 311.3 | 75.4 | 6.2 | 17.58 | 10.2 | −4.29 | 239 |
| J1400−1431 | 2015-10 | 2019-05 | 7 | 327.0 | 45.1 | 3.1 | −2.11 | 4.9 | −4.33 | 167 |
| J1607−0032 | 2013-09 | 2019-05 | 6 | 10.7 | 35.5 | 421.8 | 19.99 | 10.7 | −3.61 | 26 |
| J1645−0317 | 2013-08 | 2019-08 | 7 | 14.1 | 26.1 | 387.7 | 18.86 | 35.8 | −4.18 | 4 |
| J2145−0750 | 2013-01 | 2019-08 | 7 | 47.8 | −42.1 | 16.1 | 5.31 | 9.0 | −4.11 | 232 |
| J2317+1439 | 2012-12 | 2019-08 | 8 | 91.4 | −42.4 | 3.4 | 17.68 | 21.9 | −4.28 | 7 |
Notes. The table reports the source name, the covered time span, the number of observing sites that have been monitoring that specific source, the Galactic coordinates, the rotational spin period, the ecliptic latitude, the DM of the pulsar as measured during the general pulsar timing analysis described in Sect. 3, the decimal logarithm of the median DM uncertainty, and the number of observations used to generate the data-derived template.
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