Detection of titanium oxide in the atmosphere of a hot Jupiter. (2017)
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/10.17863/cam.23299
Publication URI: https://www.repository.cam.ac.uk/handle/1810/276018
Type: Journal Article/Review