He: Detection
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G-B: High resolution IR | Giant Tidal Tails of Helium Escaping the Hot Jupiter HAT-P-32 b2023, Zhoujian Zhang, Caroline V. Morley et al. |
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CO2: Detection H2O: Detection Rayleigh Scattering: Detection
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G-B: Low resolution visible | A Two-limb Explanation for the Optical-to-infrared Transmission Spectrum of the Hot Jupiter HAT-P-32Ab2023, Xin-Kai Li, Guo Chen et al. |
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H2O: Detection
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HST WFC3 | Five key exoplanet questions answered via the analysis of 25 hot Jupiter atmospheres in eclipse2022, Quentin Changeat, Billy Edwards et al. |
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H: Detection He: Detection
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G-B: High resolution IR | H$α$ and He I absorption in HAT-P-32 b observed with CARMENES -- Detection of Roche lobe overflow and mass loss2021, S. Czesla, M. Lampón et al. |
CARMENES observations. Hα max. depth 3.3%. He max. depth 5.3%. |
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. |
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HST STIS | The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab2020, Alam, Munazza K., López-Morales, Mercedes et al. |
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H2O: Detection
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HST WFC3 | A Population Study of Gaseous Exoplanets2018, Tsiaras, A., Waldmann, I. P. et al. |
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H2O: Detection
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HST WFC3 | Near-IR Transmission Spectrum of HAT-P-32b using HST/WFC32017, Damiano, M., Morello, G. et al. |