Image Details
Caption: Figure 4.
NEATM model fits, including distributions of Bond albedo A, visible geometric albedo pV, and diameter D. Model fits were performed on the averaged irradiance spectrum after scaling each visit to the overall flux of the final set of observations (February 15). The non-NEATM-subtracted averaged reflectance spectrum is available in machine-readable format as the data behind the figure.
© 2026. The Author(s). Published by the American Astronomical Society.