Fig. 14
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Source region for JFC-like fireballs detected by the DFN, EFN, MORP, and FRIPON determined by the NEOMOD debiased NEO model (Nesvorný et al. 2023). The source region probabilities were also determined for the near-Earth portion of the JFC population; the low JFC source region likelihood for these comets is due to the significantly higher number of asteroids from the MB in the same a-e-i region.
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