Table 4
For each model and for the observed dataset, we give from left to right the scaled numbers of pulsars visible in the radio or γ-ray band, in the radio and γ-ray bands, in γ-rays only, and the fraction of radio loud objects in the γ visible sample.
| PS R (Radio ∨ γ) | PS R (Radio ∧ γ) | PS R γ only | PSR(Radio ∧ γ)/PSRγ all | ||||||
|
|
|||||||||
| PC | 1431 | 3.6 | 0.5 | 0.87 | |||||
| SG | 1508 | 75 | 79 | 0.49 | |||||
| OG | 1496 | 123 | 66 | 0.65 | |||||
| OPC | 1524 | 107 | 94 | 0.53 | |||||
| LAT | \ | 25 | 30 | 0.45 | |||||
Notes. All the data refer to two years of LAT observations.
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