Fig. 5
Visible geometric albedos versus diameters derived here from the AKARI IRC All-sky survey fluxes (top panel), those of U11H13 (middle panel), and those computed for all our objects that were reported in the tables by Mainzer et al. (2016). The colour code is proportional to the number of points in each bin normalised to the total number of points, which is different in each case.
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