Fig. 8.
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Comparison of the derived magnetar parameters in this work (BP and Pi) with LGRBs (green triangles; Lyons et al. 2010; Yi et al. 2014), SGRBs (black squares; Rowlinson et al. 2010, 2013; Lü et al. 2015) and SLSNe (blue circles; Nicholl et al. 2017). The gray region represents the breakup limit of a neutron star, which is around 0.96 ms (Lattimer & Prakash 2004). FXTs related to the free and trapped models are represented by star and diamond markers, respectively.
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