Image Details
Caption: Figure C1.
Targets in our sample with near-infrared spectra or photometry that sufficiently sample their blackbody-like continua and allow the peak wavelength to be determined. The spectrum and photometry shown for each object (gray lines and squares) have been subtracted by the power-law component fitted to the continuum blueward of the inflection points.
© 2026. The Author(s). Published by the American Astronomical Society.