|
TOI-3884 b
|
He |
G-B: High resolution IR |
2026, Joe P. Ninan, Jessica Libby-Roberts et al. |
Asymmetric outflow morphology supports irradiation-driven mass loss |
|
V 1298 Tau b
|
He |
G-B: High resolution IR |
2026, G. Guilluy, J. Orell-Miquel et al. |
|
|
WASP-94 A b
|
CO2 H2O CO H2S Molecular ratios: C/O, etc... |
JWST-NIRSpec |
2026, Sagnick Mukherjee, Luis Welbanks et al. |
|
|
KELT-2 A b
|
CO2 H2O Molecular ratios: C/O, etc... |
G-B: High resolution IR |
2026, Yuya Hayashi, Stevanus K. Nugroho et al. |
|
|
KELT-18 b
|
He |
G-B: High resolution IR |
2026, M. Chella, M. Monticelli et al. |
|
|
WASP-17 b
|
CO2 H2O Eclipse mapping |
JWST-NIRISS |
2026, Lili Alderson, Hannah R. Wakeford et al. |
|
|
WASP-13 b
|
Featureless spectra |
G-B: High resolution IR |
2026, D. Sicilia, M. Basilicata et al. |
|
|
51 Peg b
|
|
G-B: High resolution visible |
2021, Scandariato, G., Borsa, F. et al. |
Upper limit on the albedo |
|
WASP-76 b
|
Mg+ |
HST STIS |
Astro-ph arXiv:2610.09128 |
|
|
LTT 9779 b
|
He H2O |
G-B: High resolution IR |
2026, S. Liu, F. Yan et al. |
|
|
LTT 9779 b
|
Featureless spectra Cloudy |
JWST-NIRSpec |
2026, Sarah Stamer, Diana Dragomir et al. |
|
|
LHS 3844 b
|
|
JWST-MIRI |
2026, Kimberly Paragas, Heather A. Knutson et al. |
emission spectrum resembles a blackbody shortward of 10 μm |
|
TOI-125 c
|
Featureless spectra |
JWST-NIRSpec |
2026, Yiwei Chai, Néstor Espinoza et al. |
|
|
TOI-125 b
|
Featureless spectra |
JWST-NIRSpec |
2026, Yiwei Chai, Néstor Espinoza et al. |
|
|
TOI-2431 b
|
|
HST WFC3 |
2026, Sebastian Zieba, Billy Edwards et al. |
|
|
GJ 357 b
|
|
JWST-MIRI |
2026, Merlin Zgraggen, Brice-Olivier Demory et al. |
Measurements not explained by current models |
|
eps Ind A b
|
NH3 CH4 CO2 |
JWST-MIRI |
2026, R. Kravtchenko, O. Berné et al. |
|
|
WASP-94 A b
|
He |
JWST-NIRISS |
2025, Sagnick Mukherjee, David K. Sing et al. |
Helium detection from one single point |
|
NGTS-10 Ab
|
Cloudy Atmospheric dynamics |
JWST-NIRSpec |
2026, Louis-Philippe Coulombe, Vivien Parmentier et al. |
|
|
WASP-52 b
|
H2O CO2 |
JWST-NIRSpec |
2026, JWST GO 3969 Team, Yanbo Pan et al. |
|