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Fig. 5.

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Evolution of our recovered geometric parameters for pulsar B over time measured using the FULLBAND (±0.72°) data set. The GR-predicted evolution of φ due to Geodetic precession is indicated by the black line. Dark orange shading indicates 68% range covered by the precession rate inferred from our hierarchical fit. Light orange shading includes scatter in the values of φ over time.

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