H2O: Detection CO: Detection CO2: Detection H2S: Detection Rayleigh Scattering: Upper limit CH4: Upper limit SO2: Upper limit NH3: Upper limit HCN: Upper limit
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JWST-NIRISS | Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared2026, L. Heinke, M. Min et al. |
JWST/NIRIS SOSS combined with HST/STIS observations, which indicate a tentative Rayleigh slope |
He: Upper limit
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G-B: High resolution IR | HET/HPF observations of Helium in warm, hot, and ultra-hot Jupiters2025, Jaume Orell-Miquel, Kyra Sampson et al. |
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CO2: Detection CO: Detection H2O: Detection CH4: Upper limit
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JWST-NIRSpec | Detection of CO$_2$, CO, and H$_2$O in the atmosphere of the warm sub-Saturn HAT-P-12b2025, N. Crouzet, B. Edwards et al. |
Combination of JWST+HST transmission observations. |
H2O: Upper limit CH4: Upper limit NH3: Upper limit
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G-B: Low resolution visible | Evidence for stellar contamination in the transmission spectra of HAT-P-12b2021, C. Jiang, G. Chen et al. |
Transmission spectrum affected y stellar activity |
H2O: Detection
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HST STIS | Optical to near-infrared transmission spectrum of the warm sub-Saturn HAT-P-12b2020, Ian Wong, Björn Benneke 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. |