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A Comprehensive Reanalysis of K2-18 b’s JWST NIRISS+NIRSpec Transmission Spectrum

  • Authors: Stephen P. Schmidt, Ryan J. MacDonald, Shang-Min Tsai, Michael Radica, Le-Chris Wang, Eva-Maria Ahrer, Taylor J. Bell, Chloe Fisher, Daniel P. Thorngren, Nicholas Wogan, Erin M. May, Piero Ferrari, Katherine A. Bennett, Zafar Rustamkulov, Mercedes López-Morales, David K. Sing

Stephen P. Schmidt et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Four independently reduced JWST transmission spectra of K2-18 b. NIRISS SOSS and NIRSpec G395H data sets reduced using the FIREFLy pipeline (green error bars; Z. Rustamkulov et al. 2022, 2023; Liu & Wang et al. 2025, in preparation; Wang et al. 2025, in preparation) are compared with the same data reduced with the exoTEDRF pipeline (blue error bars; A. D. Feinstein et al. 2023; M. Radica et al. 2023; M. Radica 2024) and two NIRSpec G395H reductions using the Eureka! pipeline (error bars with gray (B)/white (A) central points; T. Bell et al. 2022). NIRISS data are shown at R ≈ 25, and NIRSpec data are shown at R ≈ 100. The four reductions demonstrate broad agreement.

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