Image Details
Caption: Figure 6.
Bond albedo (AB) and heat recirculation efficiency (ϵ) χ2 surfaces of LTT 9779 b calculated from dayside and nightside effective temperature estimates, and best-fit irradiation temperature ﹩{T}_{0}=278{3}_{-38}^{+35}﹩ K. The 1σ, 2σ, and 3σ regions for each instrument are shown in a different shade. The yellow star represents the best-fit AB and ϵ as calculated from the 1000 iteration Monte Carlo simulation with the NIRSpec+NIRISS effective temperatures. Top: χ2 surfaces derived with standard errors. Bottom: χ2 surfaces calculated with errors inflated by captured flux fractions. With errors inflated by the captured flux, only the NIRSpec+NIRISS measurements remain well constrained.
© 2026. The Author(s). Published by the American Astronomical Society.