Table 1.
Overview of the radio observations.
| Pulsar | Pulsar | tspan | Nobs |
||||
|---|---|---|---|---|---|---|---|
| (disc.) | (yr) | LOFAR |
Lovell |
NRT | |||
| (c) | (i) | (P) | (L) | (L) | |||
| J0039+3546 | J0039+35 | 6.5 | 34 | 242 | 1 | 8 | 9 |
| J0059+6956 | J0059+69 | 2.4 | 33 | 3 | |||
| J0139+5621 | J0140+5622 | 7.9 | 50 | 2 | 57 | ||
| J0305+1123 | J0305+11 | 5.1 | 67 | 1 | 7 | ||
| J0317+1328 | J0317+13 | 3.1 | 37 | 1 | 3 | 1 | |
| J0613+3731 | J0613+3731 | 9.0 | 56 | 416 | 3 | 84 | |
| J0811+3729 | J0811+37 | 4.1 | 43 | 2 | 6 | 3 | |
| J0813+2202 | J0813+22 | 2.0 | 29 | 11 | 5 | ||
| J0828+5304 | J0827+53 | 2.4 | 64 | 24 | 3 | ||
| J0928+3039 | J0928+30 | 2.6 | 31 | 1 | 6 | 5 | |
| J0935+3312 | J0935+33 | 3.9 | 39 | 50 | 3 | 6 | 10 |
| J1303+3815 | J1303+38 | 1.7 | 24 | 17 | 3 | ||
| J1334+1005 | J1334+10 | 1.7 | 24 | 5 | |||
| J1427+5211 | J1426+52 | 2.4 | 34 | 14 | 5 | ||
| J1529+4050 | J1529+40 | 7.1 | 38 | 203 | 2 | 104 | 4 |
| J1707+3556 | J1707+35 | 1.9 | 25 | 3 | |||
| J1715+4603 | J1715+46 | 2.5 | 32 | 1 | 29 | 3 | |
| J1722+3519 | J1722+35 | 2.4 | 28 | 1 | 5 | 4 | |
| J1740+2715 | J1740+27 | 6.0 | 32 | 210 | 1 | 52 | 3 |
| J1745+4254 | J1745+42 | 5.8 | 52 | 1 | 49 | 2 | |
| J1809+1705 | J1809+17 | 3.0 | 41 | 1 | 8 | 3 | |
| J1814+2224 | J1814+22 | 6.8 | 33 | 258 | 1 | 77 | 1 |
| J1910+5655 | J1910+56 | 3.0 | 53 | 18 | 4 | ||
| J1953+3014 | J1953+30 | 2.4 | 34 | 46 | 4 | ||
| J1958+2214 | J1958+21 | 2.2 | 26 | ||||
| J1958+5650 | J1958+56 | 2.3 | 34 | 37 | 1 | ||
| J2006+2205 | J2006+22 | 2.7 | 32 | 1 | 5 | 6 | |
| J2022+2112 | J2022+21 | 2.0 | 28 | 5 | 3 | ||
| J2053+1718 | J2053+17 | 2.5 | 32 | 5 | 4 | ||
| J2057+2128 | J2057+21 | 3.1 | 42 | 6 | |||
| J2123+3624 | J2123+36 | 2.4 | 33 | 15 | 3 | ||
| J2209+2117 | J2209+22 | 6.2 | 33 | 121 | 3 | ||
| J2306+3124 | J2306+31 | 6.2 | 28 | 213 | 140 | 3 | |
| J2336−0151 | J2336−01 | 3.1 | 43 | 1 | 4 | 9 | |
| J2350+3140 | J2350+31 | 3.6 | 36 | 38 | 1 | 7 | 14 |
Notes. Pulsar names are provided based on the timing positions as well as the discovery designation with which they were reported in Coenen et al. (2014) and Sanidas et al. (2019) (disc.). The observation time span is given by tspan and the number of observations from the LOFAR Core (c) and International Stations (i), the Lovell telescope at 334 MHz (P-band) and 1532 MHz (L-band), and the NRT at 1484 MHz (L-band) is as indicated.
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