Detection of titanium oxide in the atmosphere of a hot Jupiter. (2017)

First Author: Sedaghati E
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