H: Upper limit
|
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
|
HST WFC3 | HST/WFC3 transmission spectroscopy of the cold rocky planet TRAPPIST-1h2022, L. J. Garcia, S. E. Moran et al. |
|
Featureless spectra: Upper limit
|
HST WFC3 | Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations2021, A. Gressier, M. Mori et al. |
IR observations with HST/WFC3 G141. Flat line is the best retrieval model. |