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JWST MEP—A World Under Spotty Starlight: Detection of CO2 and H2O in the Hot Saturn WASP-52b with JWST NIRSpec G395H

  • Authors: Yanbo Pan, 彦博 潘, Ryan J. MacDonald, Néstor Espinoza, Bibiana Prinoth, Zafar Rustamkulov, Luis Welbanks, Daniel Kitzmann, Nicolas Crouzet, Anna Walde, Diana Powell, Eva-Maria Ahrer, Adam J. Burgasser, Duncan A. Christie, Wolf Cukier, Carlos Gascón, Måns Holmberg, Thomas Kennedy, Mercedes López- Morales, N. J. Mayne, Dominic Samra, Arjun B. Savel, Maria E. Steinrueck, Christopher P. Wirth

Yanbo Pan et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

JWST NIRSpec/G395H transmission spectrum of WASP-52b. Three independent data reductions are compared: FIREFly (brown circles), the JWST default pipeline (purple triangles), and transitspectroscopy (blue stars). The Spitzer/IRAC data from M. K. Alam et al. (2018) are overplotted for comparison for the 3.6 μm and 4.5 μm filters (orange diamonds).

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