Table 2.
Millisecond pulsars detected by NenuFAR (eight of which are detected for the first time below 100 MHz – they are marked with an asterisk).
| Millisecond | Duration | S/N | DM | Mean flux |
|---|---|---|---|---|
| pulsar | (min) | (pc cm−3) | (mJy) | |
| J0030+0451 | 184 | 33 | 4.3331(1) | 67(34) |
| J0034−0534 | 178 | 46 | 13.76530(1) | 1168(584) |
| J0214+5222* | 178 | 7 | 22.0392(3) | 5(3) |
| J0740+6620* | 142 | 9 | 14.9620(1) | 6(3) |
| J1022+1001* | 178 | 52 | 10.25356(3) | 31(16) |
| J1231−1411* | 126 | 10 | 8.0918(1) | 34(17) |
| B1257+12* | 178 | 14 | 10.1539(1) | 25(13) |
| J1400−1431 | 120 | 98 | 4.93380(1) | 386(193) |
| J1658+3630* | 23 | 9 | 3.045(1) | 12(6) |
| J1710+49* | 178 | 7 | 7.0854(1) | 4(2) |
| J1806+2819* | 178 | 28 | 18.6732(1) | 30(15) |
| J2145−0750 | 178 | 50 | 9.0053(1) | 90(45) |
Notes. For each of them the observing duration in minutes, the S/N of the detection, the best-fit DM calculated using pdmp (part of the software package PSRCHIVE), and the mean flux density determined with an error bar of 50% from a bandwidth of 75 MHz centered at 50 MHz are listed.
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