A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
Journal article, 2024
A combined analysis of datasets across four JWST instrument modes provides a benchmark transmission spectrum for the Saturn-mass WASP-39 b. The broad wavelength range and high resolution constrain orbital and stellar parameters to below 1%.
Author
Aarynn L. Carter
Space Telescope Science Institute (STScI)
University of California
E. M. May
The Johns Hopkins University Applied Physics Laboratory
Néstor Espinoza
Johns Hopkins University
Space Telescope Science Institute (STScI)
Luis Welbanks
Arizona State University
Eva Maria Ahrer
Max Planck Society
The University of Warwick
L. Alderson
University of Bristol
Rafael Brahm
Data Observatory Foundation
Adolfo Ibáñez University
Millennium Institute of Astrophysics
A. D. Feinstein
University of Colorado at Boulder
University of Chicago
D. Grant
University of Bristol
Michael R. Line
Arizona State University
Giuseppe Morello
Instituto de Astrofísica de Canarias
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
R. O’Steen
Space Telescope Science Institute (STScI)
Michael Radica
Université de Montréal
Zafar Rustamkulov
Johns Hopkins University
Kevin B. Stevenson
The Johns Hopkins University Applied Physics Laboratory
Jake D. Turner
Cornell University
Munazza K. Alam
Carnegie Institution of Washington
Space Telescope Science Institute (STScI)
D. Anderson
The University of Warwick
Natalie Batalha
University of California
M. P. Battley
University of Geneva
D. Bayliss
The University of Warwick
Jacob L. Bean
University of Chicago
B. Benneke
Université de Montréal
Z. K. Berta-Thompson
University of Colorado at Boulder
Jonathan Brande
University of Kansas
E. Bryant
University College London (UCL)
Matt Burleigh
University Of Leicester
Louis Philippe Coulombe
Université de Montréal
I. J.M. Crossfield
University of Kansas
Mario Damiano
California Institute of Technology (Caltech)
J. M. Desert
Anton Pannekoek Institute for Astronomy
Laura Flagg
Cornell University
S. Gill
The University of Warwick
Julie Inglis
California Institute of Technology (Caltech)
J. Kirk
Imperial College London
California Institute of Technology (Caltech)
H. Knutson
California Institute of Technology (Caltech)
L. Kreidberg
Max Planck Society
Mercedes López-Morales
Harvard-Smithsonian Center for Astrophysics
M. Mansfield
University of Arizona
Sarah E. Moran
University of Arizona
C.A. Murray
University of Colorado at Boulder
M. C. Nixon
College of Computer, Mathematical, & Natural Sciences
Dominique J.M. Petit dit de la Roche
University of Geneva
Benjamin V. Rackham
Massachusetts Institute of Technology (MIT)
E. Schlawin
University of Arizona
David K. Sing
Johns Hopkins University
Hannah R. Wakeford
University of Bristol
N. L. Wallack
Carnegie Institution of Washington
P. J. Wheatley
The University of Warwick
Sebastian Zieba
Leiden University
Max Planck Society
Keshav Aggarwal
Indian Institute of Technology
J. Barstow
Open University
Taylor Bell
NASA Ames Research Center
Jasmina Blecic
New York University Abu Dhabi
Claudio Caceres
Núcleo Milenio de Formación Planetaria (NPF)
Universidad Andrés Bello
Centro de Astrofísica y Tecnologías Afines (CATA),
N. Crouzet
Leiden University
P. E. Cubillos
Institut fur Weltraumforschung
Istituto nazionale di astrofisica (INAF)
Tansu Daylan
Princeton University
Miguel De Val-Borro
Planetary Science Institute
L. Decin
KU Leuven
Jonathan J. Fortney
University of California
N. P. Gibson
Trinity College Dublin
Kevin Heng
The University of Warwick
Ludwig Maximilian University of Munich (LMU)
Renyu Hu
California Institute of Technology (Caltech)
Eliza M.R. Kempton
College of Computer, Mathematical, & Natural Sciences
P. O. Lagage
University Paris-Saclay
Joshua D. Lothringer
Utah Valley University
Space Telescope Science Institute (STScI)
J. Lustig-Yaeger
The Johns Hopkins University Applied Physics Laboratory
L. Mancini
Max Planck Society
University of Rome Tor Vergata
Istituto nazionale di astrofisica (INAF)
Nathan J. Mayne
University of Exeter
L. C. Mayorga
The Johns Hopkins University Applied Physics Laboratory
K. Molaverdikhani
Ludwig Maximilian University of Munich (LMU)
E. Nasedkin
Max Planck Society
K. Ohno
National Astronomical Observatory of Japan
Vivien Parmentier
Observatoire de la Cote d'Azur
Diana Powell
Harvard-Smithsonian Center for Astrophysics
S. Redfield
Wesleyan University
P. Roy
Université de Montréal
Jake Taylor
University of Oxford
Université de Montréal
Xi Zhang
University of California
Nature Astronomy
23973366 (eISSN)
Vol. 8 8 1008-1019Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.1038/s41550-024-02292-x