Fig. 6.
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Diagram of spin-down rate vs. spin period of the pulsars from the ATNF catalogue (version: 2.1.1; Manchester et al. 2005). The location of J0657 is indicated as a blue data point with error bars. We highlight the position of the ‘three musketeers’ (PSR B0656+14, Geminga, and PSR B1055–52; magenta), high magnetic field spin-powered pulsars (red; same selection as in Kurpas et al. 2024a), the ‘magnificent seven’ (green), and magnetars (orange).
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