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Thermal emission at 3.6–8 μm from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star

Anderson, D. R.; Smith, A. M. S.; Madhusudhan, N.; Wheatley, P. J.; Collier Cameron, A.; Hellier, C.; Campo, C.; Gillon, M.; Harrington, J.; Maxted, P. F. L.; Pollacco, D.; Queloz, D.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.

Authors

D. R. Anderson

A. M. S. Smith

N. Madhusudhan

P. J. Wheatley

A. Collier Cameron

C. Campo

M. Gillon

J. Harrington

D. Pollacco

D. Queloz

A. H. M. J. Triaud

R. G. West



Abstract

We report detection of thermal emission from the exoplanet WASP-19b at 3.6, 4.5, 5.8 and 8.0 μm. We used the InfraRed Array Camera on the Spitzer Space Telescope to observe two occultations of WASP-19b by its host star. We combine our new detections with previous measurements of WASP-19b's emission at 1.6 and 2.09 μm to construct a spectral energy distribution of the planet's dayside atmosphere. By comparing this with model-atmosphere spectra, we find that the dayside atmosphere of WASP-19b lacks a strong temperature inversion. As WASP-19 is an active star (log R′HK = −4.50 ± 0.03), this finding supports the hypothesis of Knutson, Howard and Isaacson that inversions are suppressed in hot Jupiters orbiting active stars. The available data are unable to differentiate between a carbon-rich and an oxygen-rich atmosphere.

Citation

Anderson, D. R., Smith, A. M. S., Madhusudhan, N., Wheatley, P. J., Collier Cameron, A., Hellier, C., …West, R. G. (2013). Thermal emission at 3.6–8 μm from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star. Monthly Notices of the Royal Astronomical Society, 430(4), 3422-3431. https://doi.org/10.1093/mnras/stt140

Journal Article Type Article
Online Publication Date Feb 20, 2013
Publication Date Apr 21, 2013
Deposit Date Jun 16, 2023
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 0035-8711
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 430
Issue 4
Pages 3422-3431
DOI https://doi.org/10.1093/mnras/stt140
Keywords Space and Planetary Science, Astronomy and Astrophysics; methods: data analysis, techniques: photometric, occultations, planets and satellites: atmospheres, planets and satellites: individual: WASP-19b, stars: individual: WASP-19