Fig. 8.
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Spin vs. spin-down diagram presenting the spin properties of the known isolated neutron star population. In the background, we plot all the objects collected in the ATNF pulsar database (Version 1.70; Manchester et al. 2005). The period of J1317 is marked by the vertical green line. The horizontal magenta line indicates the upper 3σ spin-down limit derived from the XMM-Newton and NICER observations.
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