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Fig. 3.
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Ratio of the pulsed B (λeff = 433 nm, Weff = 90 nm) luminosity to the spin-down power for J2339 (orange dot) and the sample of detected optical pulsars. The data are from Ambrosino et al. (2017, see Fig. 3, Supplementary Table 1, and references therein), Papitto et al. (2019), and Ambrosino et al. (2021).
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