Fig. D.1
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Gray: Histogram of the millisecond pulsar age distribution adopted in DPS (see Appendix D.1), with logarithmically spaced bins along the x-axis; Pink: Uniform distribution 𝒰(0.1, 13.6)(Gyr) with logarithmically spaced bins along the x-axis, which is only used to examine the DPS robustness with respect to uncertainties in the MSP age distribution (see Appendix D.2).
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