Fig. 24.
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Comparison between the unpublished period distribution of an all-sky astrometric orbit sample (top panel, blue line, same as the bottom panel of Fig. 16) and that predicted by our fits to the noiseless sampled bias model of Eq. (7) for different scan-angle harmonics k (purple lines in the following panels). See Figs. C.6 and C.7 for ecliptic sky maps of the most prominent peaks.
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