Image Details
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.
© 2026. The Author(s). Published by the American Astronomical Society.