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Fig. 4

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A single pulse search of PSR J0248+6021. For each of 250 DM values, the 96 NBPP radio frequency samples are de-dispersed and summed. Bottom frame: summed intensities with signal-to-noise 5σ above the average noise level are shown as points. Larger points indicate larger S/N. Top frames: projections showing a clear pulsar detection.

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