Fig. 13.
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Comparison of PSR B0950+08’s MP+precursor fluence distribution to the sample of normal pulsars from Mickaliger et al. (2018, light green lines) and the collection of “classical” GPs normalized to FAP (colored lines). Other measurements of the PSR B0950+08 single-pulse fluence distributions from Fig. 10 are given in gray (using the same markers as in that Figure).
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