Image Details
Caption: Figure 2.
SED of TOI 560 from the first of our two independent SED analyses; this analysis is particularly suited for the identification of the NUV excess. Red symbols represent the observed photometric measurements, where the horizontal bars represent the effective width of the passband. Blue symbols are the model fluxes from the best-fit NextGen atmosphere model (black).
© 2022. The Author(s). Published by the American Astronomical Society.