Is TiO emission present in the ultra-hot Jupiter WASP-33b? A reassessment using the improved ExoMol TOTO line list

Author(s):
Serindag, D.B. (0000-0001-7987-2079); Nugroho, S.K.; Mollière, P.; Mooij, E.J.W. de; Gibson, N.P.; Snellen, I.A.G. (0000-0003-1624-3667)
Published
2021
Publication type
Article / Letter to editor
Planets and SatellitesAtmosphereCompositionIndividualWASP-33bTechniquesSpectroscopicAstrophysicsEarth and Planetary Astrophysics
Date issued
2021
Language
English
Is part of
Astronomy and Astrophysics
hdl
1887/3251005
doi
10.1051/0004-6361/202039135
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...645A..90S