Fig. 3.
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Left: χ−ζ plane showing the best-fit couple of angles χ and ζ for the first sample of MSPs. Right: ζ − i plane showing the best-fit angle, ζ, for the inclination, i, imposed by Shapiro delay measurements, with the blue dotted line corresponding to the perfect alignment condition i = ζ. Individual pulsars are depicted by different colours.
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