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Fig. 5.

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Waterfall plots showing, for the two RB pulsars J1036−4353 and J1803−6707, orbital longitude (with respect to the ascending node) versus pulse phase. The brighter the colour-scale, the stronger the signal. Orbital longitude ranges where the plots show a solid colour have no associated data, as observations were planned to avoid the eclipses. Data are from the Parkes telescope.

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