February
2023
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2023Natur.614..670F
Authors
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Feinstein, Adina D.
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Radica, Michael
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Welbanks, Luis
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Murray, Catriona Anne
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Ohno, Kazumasa
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Coulombe, Louis-Philippe
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Espinoza, Néstor
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Bean, Jacob L.
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Teske, Johanna K.
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Benneke, Björn
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Line, Michael R.
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Rustamkulov, Zafar
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Saba, Arianna
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Tsiaras, Angelos
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Barstow, Joanna K.
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Fortney, Jonathan J.
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Gao, Peter
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Knutson, Heather A.
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MacDonald, Ryan J.
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Mikal-Evans, Thomas
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Rackham, Benjamin V.
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Taylor, Jake
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Parmentier, Vivien
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Batalha, Natalie M.
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Berta-Thompson, Zachory K.
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Carter, Aarynn L.
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Changeat, Quentin
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dos Santos, Leonardo A.
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Gibson, Neale P.
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Goyal, Jayesh M.
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Kreidberg, Laura
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López-Morales, Mercedes
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Lothringer, Joshua D.
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Miguel, Yamila
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Molaverdikhani, Karan
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Moran, Sarah E.
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Morello, Giuseppe
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Mukherjee, Sagnick
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Sing, David K.
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Stevenson, Kevin B.
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Wakeford, Hannah R.
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Ahrer, Eva-Maria
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Alam, Munazza K.
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Alderson, Lili
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Allen, Natalie H.
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Batalha, Natasha E.
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Bell, Taylor J.
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Blecic, Jasmina
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Brande, Jonathan
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Caceres, Claudio
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Casewell, S. L.
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Chubb, Katy L.
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Crossfield, Ian J. M.
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Crouzet, Nicolas
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Cubillos, Patricio E.
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Decin, Leen
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Désert, Jean-Michel
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Harrington, Joseph
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Heng, Kevin
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Henning, Thomas
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Iro, Nicolas
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Kempton, Eliza M. -R.
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Kendrew, Sarah
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Kirk, James
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Krick, Jessica
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Lagage, Pierre-Olivier
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Lendl, Monika
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Mancini, Luigi
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Mansfield, Megan
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May, E. M.
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Mayne, N. J.
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Nikolov, Nikolay K.
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Palle, Enric
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Petit dit de la Roche, Dominique J. M.
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Piaulet, Caroline
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Powell, Diana
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Redfield, Seth
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Rogers, Laura K.
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Roman, Michael T.
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Roy, Pierre-Alexis
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Nixon, Matthew C.
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Schlawin, Everett
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Tan, Xianyu
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Tremblin, P.
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Turner, Jake D.
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Venot, Olivia
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Waalkes, William C.
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Wheatley, Peter J.
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Zhang, Xi
Abstract
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The Saturn-mass exoplanet WASP-39b has been the subject of extensive efforts to determine its atmospheric properties using transmission spectroscopy1-4. However, these efforts have been hampered by modelling degeneracies between composition and cloud properties that are caused by limited data quality5-9. Here we present the transmission spectrum of WASP-39b obtained using the Single-Object Slitless Spectroscopy (SOSS) mode of the Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST. This spectrum spans 0.6-2.8 μm in wavelength and shows several water-absorption bands, the potassium resonance doublet and signatures of clouds. The precision and broad wavelength coverage of NIRISS/SOSS allows us to break model degeneracies between cloud properties and the atmospheric composition of WASP-39b, favouring a heavy-element enhancement (`metallicity') of about 10-30 times the solar value, a sub-solar carbon-to-oxygen (C/O) ratio and a solar-to-super-solar potassium-to-oxygen (K/O) ratio. The observations are also best explained by wavelength-dependent, non-grey clouds with inhomogeneous coverageof the planet's terminator.
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