Constraining the magnetic field geometry of the millisecond pulsar PSR J0030+0451 from joint radio, thermal X-ray, and γ-ray emission

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Table 4.

Time lag ϕ₁ and ϕ₂ in degrees and in units of the period, as defined in Fig. 5 and corresponding to the plot in Fig. 6.

Model	ϕ₂ (deg)	ϕ₁ (deg)	ϕ₂	ϕ₁
ST+PST	−26	8	−0.072	0.022
ST+EST	−10	6	−0.028	0.016
ST+CST	−9	6	−0.025	0.017
ST+U	−10	6	−0.027	0.015
CDT+U	−9	6	−0.026	0.017

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