WD0806 b is a rare exoplanet companion orbiting a white dwarf, currently with a projected orbital distance of 2500 au. The Spitzer mid-IR photometry suggests that the temperature is as […]
![The best-fit PICASO retrieval temperature-pressure (TP) profile is plotted as a solid blue line with the temperature-pressure knots indicated in solid blue circles. The light blue shaded region indicates the 3σ confidence interval of the retrieved TP profiles. The tightly constrained TP profiles in the 1–10 bar range match with the peak of the 3–5 µmcontribution function plotted in the right panel. The retrieved TP profile based on MIRI-LRS 5–11.7 µmspectrum in Voyer et al. (2025) is plotted in solid purple along with the 3σ uncertainty plotted as light-purple shaded region. The condensation curves of H2O, Na2S, and KCl at solar metallicity are plotted with blue, orange, and green dashed lines respectively. For reference, the solid black line shows the TP profile of the best-fit Elf Owl grid model ([M/H] = -1, C/O = 1.5, log(g) = 3.23, log(Kzz) = 7, Teff= 350 K). Right panel: The contribution function map of the best-fit PICASO retrieval results shows that most of the 3–5 µmflux is emitted from 0.1–10 bar region. -- astro-ph.EP](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/02/JWST-Spectral-Retrieval.png?resize=1200%2C719&ssl=1)
WD0806 b is a rare exoplanet companion orbiting a white dwarf, currently with a projected orbital distance of 2500 au. The Spitzer mid-IR photometry suggests that the temperature is as […]