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dc.contributor.authorFeinstein, Adina D.
dc.contributor.authorRadica, Michael
dc.contributor.authorWelbanks, Luis
dc.contributor.authorMurray, Catriona Anne
dc.contributor.authorOhno, Kazumasa
dc.contributor.authorCoulombe, Louis-Philippe
dc.contributor.authorEspinoza, Néstor
dc.contributor.authorBean, Jacob L.
dc.contributor.authorTeske, Johanna K.
dc.contributor.authorBenneke, Björn
dc.contributor.authorLine, Michael R.
dc.contributor.authorRustamkulov, Zafar
dc.contributor.authorSaba, Arianna
dc.contributor.authorTsiaras, Angelos
dc.contributor.authorBarstow, Joanna K.
dc.contributor.authorFortney, Jonathan J.
dc.contributor.authorGao, Peter
dc.contributor.authorKnutson, Heather A.
dc.contributor.authorMacDonald, Ryan J.
dc.contributor.authorMikal-Evans, Thomas
dc.contributor.authorRackham, Benjamin V.
dc.contributor.authorTaylor, Jake
dc.contributor.authorParmentier, Vivien
dc.contributor.authorBatalha, Natalie M.
dc.contributor.authorBerta-Thompson, Zachory K.
dc.contributor.authorCarter, Aarynn L.
dc.contributor.authorChangeat, Quentin
dc.contributor.authorDos Santos, Leonardo A.
dc.contributor.authorGibson, Neale P.
dc.contributor.authorGoyal, Jayesh M.
dc.contributor.authorKreidberg, Laura
dc.contributor.authorLópez-Morales, Mercedes
dc.contributor.authorLothringer, Joshua D.
dc.contributor.authorMiguel, Yamila
dc.contributor.authorMolaverdikhani, Karan
dc.contributor.authorMoran, Sarah E.
dc.contributor.authorMorello, Giuseppe
dc.contributor.authorMukherjee, Sagnick
dc.contributor.authorSing, David K.
dc.contributor.authorStevenson, Kevin B.
dc.contributor.authorWakeford, Hannah R.
dc.contributor.authorAhrer, Eva-Maria
dc.contributor.authorAlam, Munazza K.
dc.contributor.authorAlderson, Lili
dc.contributor.authorAllen, Natalie H.
dc.contributor.authorBatalha, Natasha E.
dc.contributor.authorBell, Taylor J.
dc.contributor.authorBlecic, Jasmina
dc.contributor.authorBrande, Jonathan
dc.contributor.authorCaceres, Claudio
dc.contributor.authorCasewell, S. L.
dc.contributor.authorChubb, Katy L.
dc.contributor.authorCrossfield, Ian J. M.
dc.contributor.authorCrouzet, Nicolas
dc.contributor.authorCubillos, Patricio E.
dc.contributor.authorDecin, Leen
dc.contributor.authorDésert, Jean-Michel
dc.contributor.authorHarrington, Joseph
dc.contributor.authorHeng, Kevin
dc.contributor.authorHenning, Thomas
dc.contributor.authorIro, Nicolas
dc.contributor.authorKempton, Eliza M. -R.
dc.contributor.authorKendrew, Sarah
dc.contributor.authorKirk, James
dc.contributor.authorKrick, Jessica
dc.contributor.authorLagage, Pierre-Olivier
dc.contributor.authorLendl, Monika
dc.contributor.authorMancini, Luigi
dc.contributor.authorMansfield, Megan
dc.contributor.authorMay, E. M.
dc.contributor.authorMayne, N. J.
dc.contributor.authorNikolov, Nikolay K.
dc.contributor.authorPalle, Enric
dc.contributor.authorde la Roche, Dominique J. M. Petit dit
dc.contributor.authorPiaulet, Caroline
dc.contributor.authorPowell, Diana
dc.contributor.authorRedfield, Seth
dc.contributor.authorRogers, Laura K.
dc.contributor.authorRoman, Michael T.
dc.contributor.authorRoy, Pierre-Alexis
dc.contributor.authorNixon, Matthew C.
dc.contributor.authorSchlawin, Everett
dc.contributor.authorTan, Xianyu
dc.contributor.authorTremblin, P.
dc.contributor.authorTurner, Jake D.
dc.contributor.authorVenot, Olivia
dc.contributor.authorWaalkes, William C.
dc.contributor.authorWheatley, Peter J.
dc.contributor.authorZhang, Xi
dc.date.accessioned2023-07-08T23:38:09Z
dc.date.available2023-07-08T23:38:09Z
dc.date.issued2023-02-23
dc.identifier282979739
dc.identifier87bb4477-dee5-4894-9d04-fd070ffd252c
dc.identifier85146867206
dc.identifier.citationFeinstein , A D , Radica , M , Welbanks , L , Murray , C A , Ohno , K , Coulombe , L-P , Espinoza , N , Bean , J L , Teske , J K , Benneke , B , Line , M R , Rustamkulov , Z , Saba , A , Tsiaras , A , Barstow , J K , Fortney , J J , Gao , P , Knutson , H A , MacDonald , R J , Mikal-Evans , T , Rackham , B V , Taylor , J , Parmentier , V , Batalha , N M , Berta-Thompson , Z K , Carter , A L , Changeat , Q , Dos Santos , L A , Gibson , N P , Goyal , J M , Kreidberg , L , López-Morales , M , Lothringer , J D , Miguel , Y , Molaverdikhani , K , Moran , S E , Morello , G , Mukherjee , S , Sing , D K , Stevenson , K B , Wakeford , H R , Ahrer , E-M , Alam , M K , Alderson , L , Allen , N H , Batalha , N E , Bell , T J , Blecic , J , Brande , J , Caceres , C , Casewell , S L , Chubb , K L , Crossfield , I J M , Crouzet , N , Cubillos , P E , Decin , L , Désert , J-M , Harrington , J , Heng , K , Henning , T , Iro , N , Kempton , E M -R , Kendrew , S , Kirk , J , Krick , J , Lagage , P-O , Lendl , M , Mancini , L , Mansfield , M , May , E M , Mayne , N J , Nikolov , N K , Palle , E , de la Roche , D J M P D , Piaulet , C , Powell , D , Redfield , S , Rogers , L K , Roman , M T , Roy , P-A , Nixon , M C , Schlawin , E , Tan , X , Tremblin , P , Turner , J D , Venot , O , Waalkes , W C , Wheatley , P J & Zhang , X 2023 , ' Early Release Science of the exoplanet WASP-39b with JWST NIRISS ' , Nature , vol. 614 , no. 7949 , pp. 670-675 . https://doi.org/10.1038/s41586-022-05674-1en
dc.identifier.issn0028-0836
dc.identifier.otherBibtex: 23FeRaWe
dc.identifier.otherORCID: /0000-0002-4552-4559/work/128097720
dc.identifier.urihttps://hdl.handle.net/10023/27922
dc.descriptionFunding: Support for this program was provided by NASA through a grant from the Space Telescope Science Institute. ADF acknowledges support by the National Science Foundation Graduate Research Fellowship Program under Grant No. DGE-1746045. MR acknowledges support from the National Sciences and Engineering Research Council of Canada, the Fonds de Recherche du Québec, as well as the Institut de Recherche sur les Exoplanètes.en
dc.description.abstractThe 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-39 b obtained using the SOSS mode of the NIRISS instrument on JWST. This spectrum spans 0.6–2.8 μm in wavelength and reveals multiple 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 ~10–30x 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-gray clouds with inhomogeneous coverage of the planet’s terminator.
dc.format.extent10299041
dc.language.isoeng
dc.relation.ispartofNatureen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subjectMCCen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleEarly Release Science of the exoplanet WASP-39b with JWST NIRISSen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1038/s41586-022-05674-1
dc.description.statusPeer revieweden
dc.date.embargoedUntil2023-07-09


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