Table 3.
Parameters of the mock pulsar signals injected in the data during the tests to evaluate the sensitivity thresholds and find optimum parameters for the data analysis.
| P | Mp | Mc | Pb | S | δ |
|---|---|---|---|---|---|
| (ms) | (M⊙) | (M⊙) | (h) | (mJy) | |
| 457.09 | – | – | – | 0.34 | 0.05 |
| 23.66 | – | – | – | 0.18 | 0.05 |
| 2.87 | – | – | – | 0.78 | 0.2 |
| 141.87 | 1.4 | 10 | 30 | 1.09 | 0.1 |
| 55.22 | 1.4 | 4.3 ⋅ 106 | 4320 | 0.82 | 0.1 |
| 1.92 | 1.4 | 4.3 ⋅ 106 | 4320 | 0.86 | 0.2 |
Notes. The first three pulsars are isolated, and the last three orbit companions; the first orbits a stellar mass black hole and the other two orbit Sgr A*. In the binary systems the orbital inclination is 90 degrees and the orbital phase is that with a maximum acceleration. The columns indicate the intrinsic spin period (P), pulsar mass (Mp), companion mass (Mc), orbital period (Pb), pulse-averaged flux density (S), and pulsar duty cycle (δ).
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