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Fig. 5

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Comparison between the geometric albedo derived by the stellar occultation (pV*, Shevchenko & Tedesco 2006; Lupishko 2018) and the polarimetric, photometric, and spectral properties associated with the low albedo asteroids with hydration features. Blue cross markers indicate asteroids with R^0.7+σR^0.7<1${\hat R_{0.7}} + \sigma {\hat R_{0.7}} < 1$ (i.e., Ch-type asteroids, DeMeo et al. 2009), while black circles indicate dark asteroids other than Ch-type ones. (g) Square markers indicate the asteroids whose R^2.7${\hat R_{2.7}}$ were obtained from Takir & Emery (2012); Takir et al. (2015).

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