Inferring the origins of the pulsed γ-ray emission from the Crab pulsar with ten-year Fermi-LAT data

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202038166e]

Table 4.

Joint fits of the LAT and ground-based instruments’ spectral points for the Crab pulsar at different phases.

Phase	Instruments	N₀^(a)	Γ	ϵ	χ²/d.o.f.
		(10⁻¹² cm⁻² s⁻¹ GeV⁻¹)
Full-phase	LAT and VERITAS	3.0 ± 0.5	3.41 ± 0.12	1.22 ± 0.12	3.1/6

P1_M	LAT and MAGIC	16.9 ± 2.9	3.20 ± 0.13	1.23 ± 0.14	8.6/14
P2_M		18.5 ± 2.6	2.85 ± 0.10

Notes.

^(a)

The PLSF model is assumed. It has been scaled by the inverse of the phase interval.

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