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 1.

Pulse peak phases determined from LAT phaseograms.

Energy band	Peak 1 ^(a)	Peak 2 ^(b)
(GeV)
0.06–0.6	0.997 ± 0.004	0.393 ± 0.004
0.6–6	0.998 ± 0.004	0.389 ± 0.005
6–60	0.998 ± 0.004	0.391 ± 0.005
20–500	0.003 ± 0.006	0.392 ± 0.004

Notes.

^(a)

It is calculated as the arithmetic mean of phases in 0.98–0.02 weighted by relative fluxes.

^(b)

It is calculated as the arithmetic mean of phases in 0.36–0.42 weighted by relative fluxes.

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