Fig. 2.
Scattering time in units of the pulsar period vs. the dispersion measure for the pulsars of our sample (centre plot, double-logarithmic axes). Detected slow pulsars are shown as blue stars, millisecond pulsars as magenta diamonds, and non-detections as red crosses. Right and bottom panels: (with semi-logarithmic axes) fraction of detected pulsars for each axis of the central plot.
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