Fig. 10From: Derivation of 1.064 μm normal albedos on the C-type asteroid Ryugu from laser pulse intensity measurement of the Hayabusa2 LIDAR\({E}_{\mathrm{T}}\) and \({D}_{\mathrm{T}}\). The third polynomial equation is adopted as the conversion function of the transmitted energy (thick black line). The straight blue line is previously derived by Yamada et al. (2017)Back to article page