Table E.1
Best fit parameters resulting from the joint fit of radio and γ-ray light curves of pulsar J1907+0602.
| J1907+0602 | PC | SG | OG | OPC | ||||||
|
|
||||||||||
| ln L | −368 | −957 | −353 | −580 | ||||||
| α [°] |
|
|
|
|
||||||
| ζ [°] |
|
|
|
|
||||||
| f Ω | 0.03 | 0.97 | 0.78 | 0.78 | ||||||
| Lγ [W] | 8.52 × 1026 | 3.06 × 1028 | 2.45 × 1028 | 2.44 × 1028 | ||||||
Notes.From top to bottom are listed, for each model, best fit log-likelihood value, magnetic obliquity α, observer line of sight ζ, γ-ray beaming factor fΩ, and γ-ray Luminosity. The errors on α and ζ bigger than 2 correspond to 3σ statistical error.
Notes.From top to bottom are listed, for each model, best fit log-likelihood value, magnetic obliquity α, observer line of sight ζ, γ-ray beaming factor fΩ, and γ-ray Luminosity. The errors on α and ζ bigger than 2 correspond to 3σ statistical error.
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