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The Asymmetric Limbs of HD 209458 b Observed with JWST NIRCam F322W2/F444W

  • Authors: Cathal Maguire, Eva-Maria Ahrer, Charlotte Fairman, Hannah R. Wakeford, Duncan A. Christie, James Kirk, Elspeth K.H. Lee, Evert Nasedkin, Michael Radica

Cathal Maguire et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure A2.

The morning (left) and evening (right) transmission spectra obtained for each of our reduction pipelines (detailed in Sections 2.1.1 and 2.1.2). The light curves were fit with Harmonica (see Section 3.1). The transit depths obtained from the Tiberius reduction are shown as filled squares, whereas the transit depths obtained from the Eureka! reduction are shown as unfilled diamonds. Horizontal black arrows highlight the wavelength coverage of the NIRCam F322W2 and F444W filters. No offset has been applied to the F444W values.

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