Image Details
Caption: Figure 1.
Sensitivity of synthetic transmission spectra to variations in (a) planetary temperature, (b) TiO mixing ratio, and (c) VO mixing ratio. The black points with error bars represent the transit depths binned according to the broadband transmission curves of the Johnson–Cousins and SDSS filters, shown in panel (d).
© 2026. The Author(s). Published by the American Astronomical Society.