Fig. 14.
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Survival function of the fluence distributions for two most studied GP pulsars, the Crab pulsar PSR B0531+21 and PSR B1937+21 from the works of Bhat et al. (2008, B08), Bera & Chengalur (2019, B19), Karuppusamy et al. (2010, K10), McKee et al. (2019, M19), Kinkhabwala & Thorsett (2000, K00), and Soglasnov et al. (2004, S04). The gray unfilled markers show fluences rescaled to a common frequency (1.3 GHz for the Crab and 1.4 GHz for PSR B1937+21) using broadband spectral fits from Bilous et al. (2016) and Kondratiev et al. (2018).
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