Exploring H 2 O Prominence in Reflection Spectra of Cool Giant Planets (2018)
Attributed to:
Inverse Modelling Methods for the Characterisation of Exoplanetary Atmospheres
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aabb05
Publication URI: http://dx.doi.org/10.3847/1538-4357/aabb05
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 1538-4357