A. L. Carter, E. M. May, N. Espinoza, L. Welbanks, E. Ahrer, L. Alderson, R. Brahm, A. D. Feinstein, D. Grant, M. Line, G. Morello, R. O’Steen, M. Radica, Z. Rustamkulov, K. B. Stevenson, J. D. Turner, M. K. Alam, D. R. Anderson, N. M. Batalha, M. P. Battley, D. Bayliss, J. L. Bean, B. Benneke, Z. K. Berta-Thompson, J. Brande, E. M. Bryant, M. R. Burleigh, L. Coulombe, I. J. M. Crossfield, M. Damiano, J.-M. Désert, L. Flagg, S. Gill, J. Inglis, J. Kirk, H. Knutson, L. Kreidberg, M. López Morales, M. Mansfield, S. E. Moran, C. A. Murray, M. C. Nixon, D. J. M. Petit dit de la Roche, B. V. Rackham, E. Schlawin, D. K. Sing, H. R. Wakeford, N. L. Wallack, P. J. Wheatley, S. Zieba, K. Aggarwal, J. K. Barstow, T. J. Bell, J. Blecic, C. Caceres, N. Crouzet, P. E. Cubillos, T. Daylan, M. de Val-Borro, L. Decin, J. J. Fortney, N. P. Gibson, K. Heng, R. Hu, E. M.-R. Kempton, P. Lagage, J. D. Lothringer, J. Lustig-Yaeger, L. Mancini, N. J. Mayne, L. C. Mayorga, K. Molaverdikhani, E. Nasedkin, K. Ohno, V. Parmentier, D. Powell, S. Redfield, P. Roy, J. Taylor, X. Zhang
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Mayne, L. C. Mayorga, K. Molaverdikhani, E. Nasedkin, K. Ohno, V. Parmentier, D. Powell, S. Redfield, P. Roy, J. Taylor, X. Zhang","doi":"10.1038/s41550-024-02292-x","DOIUrl":null,"url":null,"abstract":"Observing exoplanets through transmission spectroscopy supplies detailed information about their atmospheric composition, physics and chemistry. Before the James Webb Space Telescope (JWST), these observations were limited to a narrow wavelength range across the near-ultraviolet to near-infrared, alongside broadband photometry at longer wavelengths. To understand more complex properties of exoplanet atmospheres, improved wavelength coverage and resolution are necessary to robustly quantify the influence of a broader range of absorbing molecular species. Here we present a combined analysis of JWST transmission spectroscopy across four different instrumental modes spanning 0.5–5.2 μm using Early Release Science observations of the Saturn-mass exoplanet WASP-39 b. Our uniform analysis constrains the orbital and stellar parameters within subpercentage precision, including matching the precision obtained by the most precise asteroseismology measurements of stellar density to date, and it further confirms the presence of Na, K, H2O, CO, CO2 and SO2 as atmospheric absorbers. Through this process, we have improved the agreement between the transmission spectra of all modes, except for the NIRSpec PRISM, which is affected by partial saturation of the detector. This work provides strong evidence that uniform light curve analysis is an important aspect to ensuring reliability when comparing the high-precision transmission spectra provided by JWST. A combined analysis of datasets across four JWST instrument modes provides a benchmark transmission spectrum for the Saturn-mass WASP-39 b. 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A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
Observing exoplanets through transmission spectroscopy supplies detailed information about their atmospheric composition, physics and chemistry. Before the James Webb Space Telescope (JWST), these observations were limited to a narrow wavelength range across the near-ultraviolet to near-infrared, alongside broadband photometry at longer wavelengths. To understand more complex properties of exoplanet atmospheres, improved wavelength coverage and resolution are necessary to robustly quantify the influence of a broader range of absorbing molecular species. Here we present a combined analysis of JWST transmission spectroscopy across four different instrumental modes spanning 0.5–5.2 μm using Early Release Science observations of the Saturn-mass exoplanet WASP-39 b. Our uniform analysis constrains the orbital and stellar parameters within subpercentage precision, including matching the precision obtained by the most precise asteroseismology measurements of stellar density to date, and it further confirms the presence of Na, K, H2O, CO, CO2 and SO2 as atmospheric absorbers. Through this process, we have improved the agreement between the transmission spectra of all modes, except for the NIRSpec PRISM, which is affected by partial saturation of the detector. This work provides strong evidence that uniform light curve analysis is an important aspect to ensuring reliability when comparing the high-precision transmission spectra provided by JWST. 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%.
Nature AstronomyPhysics and Astronomy-Astronomy and Astrophysics
CiteScore
19.50
自引率
2.80%
发文量
252
期刊介绍:
Nature Astronomy, the oldest science, has played a significant role in the history of Nature. Throughout the years, pioneering discoveries such as the first quasar, exoplanet, and understanding of spiral nebulae have been reported in the journal. With the introduction of Nature Astronomy, the field now receives expanded coverage, welcoming research in astronomy, astrophysics, and planetary science. The primary objective is to encourage closer collaboration among researchers in these related areas.
Similar to other journals under the Nature brand, Nature Astronomy boasts a devoted team of professional editors, ensuring fairness and rigorous peer-review processes. The journal maintains high standards in copy-editing and production, ensuring timely publication and editorial independence.
In addition to original research, Nature Astronomy publishes a wide range of content, including Comments, Reviews, News and Views, Features, and Correspondence. This diverse collection covers various disciplines within astronomy and includes contributions from a diverse range of voices.