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Table 1.
Parameters used for individual simulations of sources selected by their CF.
| Definition | Parameter | Example 1 | Example 2 |
|---|---|---|---|
| Pulsar injection: | |||
| Initial period | P0 [s] | 0.10 | 0.07 |
| Initial period derivative | Ṗ0 [s s−1] | 4.3 × 10−12 | 1.5 × 10−12 |
| Initial spin-down luminosity | L0 [erg s−1] | 1.6 × 1038 | 1.6 × 1038 |
| Initial spin-down age | τ0 [yr] | 5.7 × 102 | 1.1 × 103 |
| Final period | P [s] | 1.81 | 0.95 |
| Final period derivative | Ṗ [s s−1] | 1.6 × 10−12 | 6.4 × 10−13 |
| Current age | tfinal [yr] | 2.5 × 104 | 3.4 × 104 |
| Environment: | |||
| SN explosion energy | ESN [×1051 erg] | 0.98 | 0.72 |
| ISM density | nISM [cm−3] | 1.09 | 0.22 |
| Ejected mass | Mej [M⊙] | 11.72 | 7.65 |
| Distance | D [kpc] | 13.5 | 10.9 |
| Spectral model: | |||
| Energy break | γb | 3.4 × 105 | 4.7 × 106 |
| Low-energy index | α1 | 1.19 | 1.24 |
| High-energy index | α2 | 2.14 | 2.46 |
| Containment factor | RL/RTS | 0.45 | 0.86 |
| Magnetic fraction | η | 0.0138 | 0.0014 |
| FIR energy density | ωFIR [eV cm−3] | 1.92 | 0.99 |
| NIR energy density | ωNIR [eV cm−3] | 1.38 | 2.76 |
| Derived quantities: | |||
| Reverberation age | tbeg, rev [yr] | 4.5 × 103 | 5.2 × 103 |
| Compression factor | Rmax/Rmin | 50.31 | 5.85 |
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