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First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b

  • Authors: Lennart van Sluijs, Emily Rauscher, Eliza M.-R. Kempton, Thomas Kennedy, Isaac Malsky, Noriyuki Matsunaga, Michael Meyer, Andrew McWilliam, John D. Monnier, Shogo Otsubo, Yuki Sarugaku, Tomomi Takeuchi

Lennart van Sluijs et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 6.

S/N as a function of system velocity (vsys) and Keplerian velocity (Kp) when combining all out-of-eclipse phases for both nights in the barycentric rest frame. The literature values for vsys and Kp are indicated by the white dashed cross. The maximum S/N is marked by the small circle, and its value is annotated at the top of the plot. Top left: for the fiducial spectral template. Top right: for the neutral iron (Fe) spectral template using the chemical profile assuming equilibrium chemistry. Bottom: the fiducial spectral template without neutral iron.

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