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Table 2
Expected (computed with Eq. (3)) over obtained signal-to-noise ratios (S/N) for the four known pulsars.
| Pulsar name | (S/N)expected | (S/N)obtained |
|
|
|
|||
| PA USB | |||
| B0329+54 | 9241.2 | 179.1 | 51.60 |
| B1937+21 | 169.81 | 31.3 | 5.43 |
| B2022+50 | 64.737 | 28.9 | 2.24 |
| B2035+36 | 32.219 | 18.3 | 1.76 |
| PMT USB | |||
| B0329+54 | 9618.6 | 191.1 | 50.33 |
| B1937+21 | 158.33 | 49.8 | 3.48 |
| B2022+50 | 64.737 | 28.8 | 2.25 |
| B2035+36 | 32.884 | 18.5 | 1.78 |
| PMT LSB | |||
| B0329+54 | 8606.1 | 167.5 | 51.38 |
| B1937+21 | 141.27 | 64.3 | 2.40 |
| B2022+50 | 59.499 | 11.8 | 5.04 |
| B2035+36 | 30.181 | 12.3 | 2.45 |
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