From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context

Vivien Parmentier; Mike R. Line; Jacob L. Bean; Megan Mansfield; Laura Kreidberg; Roxana Lupu; Channon Visscher; Jean-Michel Désert; Jonathan J. Fortney; Magalie Deleuil; Jacob Arcangeli; Adam P. Showman; Mark S. Marley

doi:10.1051/0004-6361/201833059

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Volume 617 (September 2018)

A&A, 617 (2018) A110

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Table 2

Blackbody temperatures based on HST/WFC3 data.

Planet	WFC3 data source	Blackbody temp. (K)^a
CoRot-2b	Wilkins et al. (2014)	1705 ± 15
HAT-P-7b	Mansfield et al. (2018)	2693 ± 14
HAT-P-32Ab	Nikolov et al. (2018)	1855 ± 16
HD 189733b	Crouzet et al. (2014)	1420 ± 4
HD 209458b	Line et al. (2016)	1601 ± 13
Kepler-13Ab	Beatty et al. (2017b)	2893 ± 19
TrES-3b	Ranjan et al. (2014)	1801 ± 39
WASP-4b	Ranjan et al. (2014)	1984 ± 26
WASP-12b	Stevenson et al. (2014a)	2894 ± 19
WASP-18b	Arcangeli et al. (2018)	2818 ± 4
WASP-33b	Haynes et al. (2015)	2801 ± 5
WASP-43b	Kreidberg et al. (2014)	1683 ± 6
WASP-103b	Kreidberg et al. (2018)	2932 ± 8
WASP-121b	Evans et al. (2017)	2650 ± 10

Notes. ^(a) The uncertainties do not take into account the uncertainty in the stellar effective temperature, which can be larger than the uncertainty derived from the data. The use of different stellar parameters/models can be a source of discrepancy with previous studies.

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