Table 4
List of the seven known pulsars redetected by the NPBS.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
|---|---|---|---|---|---|---|---|---|
| PSR | P0 (ms) | DM (pc cm−3) | P0 ,meas (ms) | DMmeas (pc cm−3) | S/N0 | θ (°) | S/Nexp | Sσ• |
| B0450+55 | 340.73 | 14.590 | 340.74 | 14.60 | 23.7 | 0.714 | 12.3 | 16.6 |
| B0655+64 | 195.67 | 8.774 | 587.17(*) | 8.77 | 20.0 | 0.173 | 19.2 | 14.1 |
| B0809+74 | 1292.24 | 5.751 | 1292.27 | 5.75 | 204.0 | 0.649 | 118.3 | 215.3 |
| B1112+50 | 1656.44 | 9.186 | 1656.48 | 9.19 | 11.7 | 0.207 | 11.1 | 57.6 |
| B1508+55 | 739.68 | 19.619 | 739.69 | 19.61 | 181.8 | 0.428 | 143.4 | 131.1 |
| B1811+40 | 931.09 | 41.557 | 931.02 | 41.57 | 10.0 | 0.757 | 4.8 | 6.9 |
| B1839+56 | 1652.86 | 26.772 | 1652.84 | 26.77 | 61.8 | 0.410 | 49.8 | 107.8 |
Notes. (1) Period in the literature (Manchester et al. 2005). (2) Dispersion measure in the literature. (3) Period of the corresponding best candidate. (4) Dispersion measure of the corresponding best candidate. (5) Expected S/N at the centre of the pointing. (6) Angular separation between the position of the pulsar and the centre of the closest digital pointing. (7) Expected S/N taking the sensitivity loss due to the angular separation into account. (8) Significance computed by PREPFOLD for the best candidate. (*)Detection of the harmonic three of B0655+64.
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