arXiv · 1904.05976
Developing a vision for exoplanetary transit spectroscopy: a shared window on the analysis of planetary atmospheres and of stellar magnetic structure
Abstract
We describe how the accurate characterization of exoplanetary atmospheres in the ELT and JWST era will inevitably require taking into consideration the stellar inhomogeneities caused by convection and magnetic fields. The existing evidence that demonstrates the mixture of stellar and planetary signatures in observed transiting spectra is presented. Finally, we discuss how to disentangle these two components through a multipronged approach that includes new solar reference spectra, improved MHD modeling, and synergistic collaborations between the communities involved, from solar to stellar and exoplanet astronomers.
Explore related subjects
Keep this discovery
Adam F. Kowalski, Karel Schrijver, Valentin Martinez Pillet, Serena Criscuoli. 2019-04-11. Developing a vision for exoplanetary transit spectroscopy: a shared window on the analysis of planetary atmospheres and of stellar magnetic structure. https://arxiv.org/abs/1904.05976
Cite the original work for its findings. Save a collection to share your selection of sources.