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GJ 436b (hot Neptune)
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Stevenson+(2010): CO, H2O,
CO2, CH4
Madhusudhan+(2011): CO, H2O,
CO2, CH4
Line+(2014): CO, H2O,
CO2, CH4
Cridland+(2016): CO
Mukherjee+(2025): CO2(2&sigma, tent)
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GJ 3090b (sub-Neptune)
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Parker+(2025): CH4(nd),
H2O(nd), NH3(nd), H2S(nd)
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HAT-P-14b (WASP-27b) (super-Jupiter)
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Liu+(2025): H2O(3.9σ)
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HD 80606 b (hot Jupiter)
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Coming Soon...
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HD 189733b (hot Jupiter)
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Grillmair+(2007): H2O(nd),
CH4(nd)
Tinetti+(2007): H2O
Swain+(2008): CH4, H2O
de Kok+(2013): CO(5σ), H2O(nd),
CO2(nd), CH4(nd)
Birkby+(2013): H2O(4.8σ),
H2O+CO2(5.1σ)
Brogi+(2016): CO+H2O(7.6σ)
Brogi+(2018): H2O(5.5σ)
Alonso-Floriano+(2019): H2O(S/N=6)
Cabot+(2019): H2O(4.8σ),
CO(4.7σ), HCN(5.0σ)
Flowers+(2019): CO+H2O(8.2σ)
Boucher+(2021): H2O(5.9σ)
Finnerty+(2024): H2O(-1.7†),
CO(-1.8†), CH4(-7.4†), NH3(-4.8†), HCN(-5.8†),
H2S(-7.7†), 13CO(~3σ)
Inglis+(2024): SiO2(s),
H2O, H2S
Zhang+(2025): H2O, CO2, CO,
H2S
†=log mass-mixing ratio
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HD 209458b (hot Jupiter)
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Swain+(2009): H2O, CH4,
CO2
Snellen+(2010): CO
Lenz+(2016):
H+
3(nd)
Brogi+(2017): CO, H2O(?)
Giacobbe+(2021): H2O(9.6&sigma,8.2σ),
CO(5.5σ), HCN(9.9σ), CH4(5.6σ,3.7σ), NH3(5.3σ,5.1σ),
C2H2(6.1σ,5.9σ,3.3σ), CO2(nd)
Hawker+(2018): H2O(S/N=4.4), CO(S/N=5.1),
H2O+CO(S/N=5.3), HCN(S/N=4.7)
Cassasaya-Barris+(2021): TiO(nd), VO(nd)
Xue+(2024): H2O, CO2,
H2S(?), CH4(nd,<-5.6†), NH3(nd,<-4.2†),
C2H2(nd,<-5.7†), HCN(nd,<-5.2†)
Blain+(2024): H2,
C2H2(nd), CH4(nd), CO(nd), CO2(nd), H2S(nd),
HCN(nd), NH3(nd)
†=log mass-mixing ratio
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HIP 99770b (super Jupiter)
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Zhang+(2024): H2O(S/n=14),
CO(S/N=23), NH3(nd), CH4(nd), 13CO(nd), CO2(nd),
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KELT-20b (MASCARA-2b) (ultra-hot Jupiter)
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Fu+(2022): H2O, CO
Nugroho+(2020): NaH(nd), MgH(nd), AlO(nd),
SH(nd), CaO(nd), VO(nd), FeH(nd), TiO(nd)
Kesseli+(2020): FeH(S/N~3)
Johnson+(2023): VO(nd,<4σ),
TiO(nd,<4σ), FeH(nd,<4σ), CaH(nd,<4σ)
Petz+(2024): VO(nd,S/N<3.4), CaH(nd,S/N<2.4),
TiO(nd,S/N<2.6), NaH(nd,S/N<2.1), MgH(nd,S/N<1.8)
Finnerty+(2025): CO, H2O
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LTT 3780c (TOI-732c) (sub-Neptune)
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Cabot+(2024): CH4(2.2σ),
NH3(nd)
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τ Boötis Ab (hot Jupiter)
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Lockwood+(2014): H2O
Pelletier+(2021): CO(-2.46‡),
H2O(nd,<-5.66‡), CH4(nd,<-3.78‡), CO2(nd,<-3.99‡),
HCN(nd,<-5.37‡), TiO(nd,<-7.54‡), C2H2(nd,<-4.88‡),
NH3(nd,<-6.10‡)
Webb+(2022): H2O(-3.3‡),
Panwar+(2022): CO(-3.44‡),
H2O(-5.13‡)
‡=log volume-mixing ratio
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TOI-5205b Jupiter-like
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Coming Soon...
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WASP-39b (hot Jupiter)
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Wakeford+(2018): H2O
Ahrer+a(2023): CO2(26σ)
Ahrer+b(2023): H2O, CH4(nd)
Rustamkulov+(2023): H2O(33σ),
CO2(28&sigma), CO(7&sigma), CH4(nd), SO2(2.7σ)
Alderson+(2023): CO2(28.5σ),
H2O(21.5σ), SO2(4.8σ)
Powell+(2024): SO2, H2O
Carter+(2024):, H2O, CO, CO2,
SO2
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WASP-80b (hot Jupiter)
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Sedaghati+(2017): H2O(nd),
CO(nd), CH4(nd)
Carleo+(2022): H2O(7.52σ),
CH4(4.17σ), NH3(4.96σ), HCN(4.11σ), CO2(tent,4.45σ),
C2H2(nd,3.39σ), CO(nd,4.62σ)
Bell+(2023): CH4(>6σ)
Richey-Yowell+(2025): H3+(nd)
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WASP-107b (warm Neptune)
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Kriedberg+(2018): H2O(6.7σ)
Dyrek+(2024): H2O(12σ),
SO2(9σ), silicate(7σ), H2S(4σ), NH3(2-3σ),
CO(2-3σ), CH4(nd)
Welbanks+(2024): CO2(29σ),
H2O(21σ), SO2(9σ), CO(7σ), NH3O(6σ),
CH4(5σ)
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WASP-121b (ultra-hot Jupiter)
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Evans+(2016): H2O(5.4σ),
TiO, VO
Evans+(2017): H2O(5σ),
TiO, VO
Tsiaras+(2018): H2O, TiO,
VO
Mikal-Evans+(2019): VO(nd?)
Merritt+(2020): TiO(nd), VO(nd)
Goyal+(2020): H2O, VO
Ouyanng+(2023): H2O, TiO, VO
Hoejmakers+(2024): TiO(nd), VO(nd)
Wardenier+(2024): H2O, CO
Pelletier+(2025): H2O, CO
Gapp+(2025): SiO(5.2σ)
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WASP-122b (KELT-14b) (hot Jupiter)
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Stangret+(2024): FeH(nd), H2O(nd),
TiO(nd), VO(nd)
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