Featureless spectra: Detection Phase curve: Yes Dayside Temperature (occultation): 369 K |
JWST-MIRI | First JWST thermal phase curves of temperate terrestrial exoplanets reveal no thick atmosphere around TRAPPIST-1 b and c2025, Michaël Gillon, Elsa Ducrot et al. |
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H: Upper limit
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HST STIS | Hubble's Multi-Year Search for Exospheres in the TRAPPIST-1 System Reveals Frequent Microflares2025, David Berardo, Julien de Wit et al. |
Lya is not very constrained due to the effect of microflares in the out-of-transit baseline, transit depth <20% at 5σ |
Featureless spectra: Detection
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JWST-NIRSpec | Stellar Contamination Correction Using Back-to-Back Transits of TRAPPIST-1 b and c2024, Alexander D. Rathcke, Lars A. Buchhave et al. |
This method enables epoch-specific stellar contamination corrections |
Featureless spectra: Detection
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JWST-NIRISS | Promise and Peril: Stellar Contamination and Strict Limits on the Atmosphere Composition of TRAPPIST-1c from JWST NIRISS Transmission Spectra2024, Michael Radica, Caroline Piaulet-Ghorayeb et al. |
Limits on the posible atmospheric compositions |
Phase curve: Yes Dayside Temperature (occultation): 380 K |
JWST-MIRI | No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c2023, Zieba, Sebastian, Kreidberg, Laura et al. |