Emission properties and bidrifting subpulses in pulsar PSR J0815+0939

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Table 1

Details of the bidrifting subpulses in PSR J0815+0939, including the observed drift properties and the associated width for each component region, are given in sector I (Szary & van Leeuwen 2017).

I. Observation				II. Simulation		III. Emission properties

Region	∆ψ°	P₃(P₁)	Drift rate (° s⁻¹)	P₃(P₁)	Drift rate (° s⁻¹)	m	y	ρ_sn(ρ_GJ)
A	24	16.62 ± 0.31	−0.5 ± 0.1	18.1 ± 3.8	−0.50 ± 0.06	25 ± 4	0.0003 ± 0.0001	0.999 ± 0.001
B	25		1.11 ± 0.04	16.6±1.7	1.11 ± 0.07	24±3	0.003 ± 0.001	0.997 ± 0.001
C	33		−0.59 ± 0.07	16.9 ± 2.6	−0.59 ± 0.01	12±2	0.004 ± 0.001	0.997 ± 0.001
D	30		−0.87 ± 0.06	17.4±1.9	−0.87 ± 0.04	10±2	0.003 ± 0.001	0.997 ± 0.001

Notes. The simulated P₃ and drift rate for each component region are given in sector II. The corresponding weighted m (rounded to the nearest integer), y, and the associated charge density, are given in sector III, with ρ_sn expressed in units of the Goldreich–Julian value.

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