Instrument calibration of the Hayabusa near-infrared spectrometer
Instrument calibration of the Hayabusa near-infrared spectrometer
Instrument calibration of the Hayabusa near-infrared spectrometer
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Figure 10: Comparison <strong>of</strong> <strong>the</strong> derived geometric albedo <strong>of</strong> Itokawa between <strong>the</strong> NIRS andAMICA. The value at V-band (0.55 μm) has been estimated by AMICA (Ishiguro et al.,2007). As an intermediary <strong>the</strong> visible to <strong>near</strong>-<strong>infrared</strong> spectra <strong>of</strong> Itokawa obtained from <strong>the</strong>ground-based observations by Binzel et al. (2001) and Tholen (2006) are plotted withnormalized at <strong>the</strong> value <strong>of</strong> AMICA’s V-band.21