Fig. 4.
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Predicted 0.5−12 keV X-ray light curve from the IBS region of PSR J1932+2121. The gray band represents the orbital phase range of the eclipse, and the purple shaded region indicates the flux uncertainty due to the distance range estimated by Misra et al. (2025). The central solid curve corresponds to the calculation with the adopted average distance of 3.3 kpc.
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