Skip to main content
Earth, Planets and Space
Fig. 5 | Earth, Planets and Space

Fig. 5

From: An evaluation method of reflectance spectra to be obtained by Hayabusa2 Near-Infrared Spectrometer (NIRS3) based on laboratory measurements of carbonaceous chondrites

Fig. 5

Data correction process of reflectance spectrum of Y-86720 meteorite. NIRS3 reflectance data were corrected for the systematic offsets of pixel signals (broken line) and further corrected using the fitting parameters calculated from the signal intensity of pixel 29 (Fig. 3). The corrected spectrum (thick solid line) is very similar to the FT-IR spectrum (thin solid line)

Back to article page