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Long-term Mid-infrared Photometry and Spectroscopy of (1) Ceres with SOFIA FORCAST

  • Authors: Anicia Arredondo, Aaron P. Deleon, Tracy M. Becker, Maggie M. McAdam

Anicia Arredondo et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure A2.

Comparison between original emissivity (gray lines, same as Figure 3) and emissivity found by scaling the flux to a SED found with constant η (colored lines). The calculated slope is visualized with a gray and cyan line, respectively, and the slope values are printed in corresponding colors. The shape of the spectra is the same, but the overall emissivity and relative slope differ. A comparison between the two methods is visualized in Figure 8.

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