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

Open Access

Table 1.

Best-fitting parameters of the trial distributions of P(log₁₀η_rad) for different distributions of distance uncertainty.

P(log₁₀η_rad)	Distance uncertainty	$η_{rad}^{peak}$ $\eta_{\mathrm{rad}}^{\mathrm{peak}}$	Std dev
𝒩	P(Δ) = 𝒩(0,0.341)	5.8%	0.42
$SN$ ${\cal SN}$	P(Δ) = 𝒩(0,0.341)	14.8%	0.47
𝒩	P(ϵ_d) = 𝒩(1,0.556)	7.2%	0.46
𝒩	P(ϵ_d) = 𝒩(1,0.2)	6.6%	0.56
𝒩	P(ϵ_d) = 𝒩(1,0.7)	7.1%	0.42

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.