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Fig. 6

image

(BR) colors vs. HR(α) absolute magnitude (uncorrected for phase effects) for all objects in our database. Centaurs and KBOs are indicated with different symbols. Haumea family objects and the two retrograde objects are also highlighted. The -shape reported by Peixinho et al. (2012) is clearly visible, and faint object bimodality is detected for , but at 2.8σ level (p-value = 0.0046).

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