The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve

@article{Deline2022TheAA,
  title={The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve},
  author={Adrien Deline and Matthew J. Hooton and Monika Lendl and Brett M. Morris and S'ebastien Salmon and Goeran Olofsson and Christopher Broeg and David Ehrenreich and M. Beck and Alexis Brandeker and Sergio Hoyer and Sophia Sulis and Val{\'e}rie Van Grootel and Vincent Bourrier and Olivier D. S. Demangeon and B-O. Demory and Kevin Heng and Hannu Parviainen and Luisa Maria Serrano and V. Singh and A. Bonfanti and L. Fossati and Daniel Kitzmann and S{\'e}rgio G. Sousa and Thomas G. Wilson and Yann Alibert and Rosa M. Alonso and Guillem Anglada and Tamas B'arczy and David Barrado y Navascu{\'e}s and Susana C. C. Barros and Wolfgang Baumjohann and Thomas Beck and Anja Bekkelien and W. Benz and Nicolas Billot and Xavier Bonfils and J. Cabrera and S{\'e}bastien Charnoz and Andrew Collier Cameron and Carlos Corral van Damme and Szil{\'a}rd Csizmadia and Melvyn B. Davies and Magali Deleuil and Laetitia Delrez and T. D. Roche and Alex Erikson and Andrea Fortier and Malcolm Fridlund and David Futyan and Daniela Gandolfi and Micha{\"e}l Gillon and Manuel Gudel and Paul E. Gutermann and J. Hasiba and Kate Gudrun Isaak and L{\'a}szl{\'o} L. Kiss and Jacques Laskar and Alain Lecavelier des Etangs and Cristophe Lovis and Demetrio Magrin and P. F. L. Maxted and Matteo Munari and Valerio Nascimbeni and Roland Ottensamer and Isabella Pagano and E. Pall'e and Gisbert Peter and Giampaolo Piotto and Don Pollacco and D. Queloz and R. Ragazzoni and Nicola Rando and Heike Rauer and Ignasi Ribas and N. C. Santos and Gaetano Scandariato and Damien S'egransan and Attila E. Simon and A M S Smith and Manfred Steller and Gy. M. Szab'o and Nicolas Thomas and St{\'e}phane Udry and Ingo Walter and Nicholas Walton},
  journal={Astronomy \& Astrophysics},
  year={2022}
}
Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperatures that are comparable to those of the coldest stars. These ‘ultra-hot Jupiters’ have atmospheres made of ions and atomic species from molecular dissociation and feature strong day-to-night temperature gradients. Photometric observations at different orbital phases provide insights on the planet’s atmospheric properties. Aims. We aim to analyse the photometric observations of WASP-189 acquired… 

References

SHOWING 1-9 OF 9 REFERENCES
Physics, Formation and Evolution of Rotating Stars
Light scattering in planetary atmospheres
This paper reviews scattering theory required for analysis of light reflected by planetary atmospheres. Section 1 defines the radiative quantities which are observed. Section 2 demonstrates the
MNRAS, in press
  • 2019
A&A, in press, https://doi
  • Mazeh,
  • 2003
Light Scattering in Planetary Atmospheres, International Series of Monographs in Natural Philosophy (Pergamon
  • 2008
Correlation plot of the parameters of the planet model made with the code corner (Foreman-Mackey 2016)
  • 2016
Transiting Planets, ed
  • ApJ, 729,
  • 2011
Light scattering in planetary atmospheres, International series of monographs in natural philosophy
  • 1975
A&A proofs: manuscript no. paper