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Exploring H 2 O Prominence in Reflection Spectra of Cool Giant Planets (2018)

First Author: MacDonald R

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