Image Details
Caption: Figure 7.
Consistency of Sonora Flame Skimmer cloud-free atmospheric models with NIRCam 5σ upper limit. Each column considers models at a different temperature (150 K, 175 K, 200 K). The top row of models corresponds to a puffy Jupiter scenario (g = 17 m s−2) and the bottom row of models corresponds to a Jupiter-like scenario (g = 31 m s−2). A red “×” indicates the model (with given [M/H] and log Kzz, where we note that log Kzz = 0 dex corresponds to a chemical equilibrium model for notational convenience) is inconsistent with (brighter than) the NIRCam 5σ upper limit. A green “✓” indicates the model is consistent with (fainter than) the NIRCam upper limit.
© 2026. The Author(s). Published by the American Astronomical Society.