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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 1.

Left panel: phase coverage of WASP-189 b’s orbit during our two observing nights. The orbit of WASP-189 b is shown face-on (dotted black line), with the observer’s direction indicated. Relative orbital phases (ϕ) are annotated along quarterly intervals. The first (green) and second (wine red) nights cover the pre-eclipse and post-eclipse phases. Both nights cover (part of) the secondary eclipse. Right panel: time series of three observables: the signal-to-noise rate per frame pair (S/N), FWHM of the trace on the detector (in pixels), and airmass are shown. The same colors as in the left panel are used to indicate each night. The time series has been binned (10 frames per bin), and the standard deviation of each bin is plotted as the shaded region.

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