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Fig. 5
Simulated evolution of 
based on a sample of 4000 clones of the observed NEJFCs by assuming that the clones are discovered at any time when their q is smaller than 1.05 AU (top panel) or decreases to 1.05 AU for the first time (bottom panel). The time is relative to the discovery epoch of the corresponding comet.
This figure is made of several images, please see below:
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