Image Details
Caption: Figure 10.
Comparison of the observed ZTF0038B spectrum (black) with archival JWST PRISM spectra of mid- to late-T dwarfs (S. A. Beiler et al. 2024). We uniformly scale the archival spectra to minimize the chi-squared statistic across the entire wavelength range (left) and across the J, H, and K bands only (right).
© 2026. The Author(s). Published by the American Astronomical Society.