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Earth, Planets and Space
Fig. 4 | Earth, Planets and Space

Fig. 4

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

Fig. 4

Correlations among the signal intensity of pixel number 29, and the inclination and y-intercept values obtained by the linear regression analyses of NIRS3 and FT-IR reflectance data (e.g., Fig. 2b). The signal intensity is normalized by integration time. All meteorite data recorded by NIRS3 are used in a, but the data of Allende are excluded in b

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