Why is it So Hot in Here? Exploring Population Trends in $\textit{Spitzer}$ Thermal Emission Observations of Hot Jupiters using Planet-Specific Self-Consistent Atmospheric Models (2022)
Attributed to:
A comprehensive study of stars, disks and exoplanets
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2201.02086
Publication URI: https://arxiv.org/abs/2201.02086
Type: Other