Rayleigh Scattering: Upper limit
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G-B: Low resolution visible | Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b2026, Napaporn A-thano, Supachai Awiphan et al. |
Transmission spectrum build from multi-color transits. Slope origin is not clear, planet or contamination |
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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He: Upper limit
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G-B: High resolution IR | Homogeneous search for helium in the atmosphere of 11 gas giant exoplanets with SPIRou2023, R. Allart, P. -B. Lemée-Joliecoeur et al. |
3sigma upper limit of <1.56 % with SPIRou |