The dispersion in pulsar γ-ray efficiency | Astronomy & Astrophysics (A&A)

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Table A.1.

Best-fitting parameters of log₁₀η_rad with P(log₁₀η_rad) = 𝒩 and P(Δ) = 𝒩(0,0.341) for the distance uncertainty, considering the original log₁₀η_obs distribution or the ones de-trended with the correlation ∝ Ė^β.

log₁₀η_obs distribution	log₁₀η_obs std dev	$η_{rad}^{peak}$ $\eta_{rad}^{peak}$	log₁₀η_rad std dev
Original	0.66	5.8%	0.42
De-trended, β = −0.50	0.60	6.6%	0.34
De-trended, β = −0.32	0.57	6.5%	0.29

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