H2O: Detection
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G-B: High resolution IR | Cross-correlation transmission spectroscopy of ultra-hot Jupiters WASP-189b, HAT-P-57b, KELT-17b, and KELT-21b with GIANO-B2026, P. Meni-Gallardo, J. Orell-Miquel et al. |
Tentative detection of water with 3.8 sigma |
He: Upper limit
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G-B: High resolution IR | The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres. No evidence of enhanced evaporation in young planets2024, J. Orell-Miquel, F. Murgas et al. |
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Featureless spectra: Detection
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G-B: Low resolution visible | Featureless transmission spectra of 12 giant exoplanets observed by GTC/OSIRIS2023, C. Jiang, G. Chen et al. |
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H: Upper limit Fe: No detection
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G-B: High resolution visible | High-resolution transmission spectroscopy study of ultra-hot Jupiters HAT-P-57b, KELT-17b, KELT-21b, KELT-7b, MASCARA-1b, and WASP-189b2021, M. Stangret, N. Casasayas-Barris et al. |
H upper limit of 0.7±0.2%. |
FeH: Upper limit
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G-B: High resolution IR | A Search for FeH in Hot-Jupiter Atmospheres with High-dispersion Spectroscopy2020, Kesseli, Aurora Y., Snellen, I. A. G. et al. |