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Diagnosing Limb Asymmetries in Hot and Ultrahot Jupiters with High-resolution Transmission Spectroscopy

  • Authors: Arjun B. Savel, Eliza M.-R. Kempton, Emily Rauscher, Thaddeus D. Komacek, Jacob L. Bean, Matej Malik, Isaac Malsky

Arjun B. Savel et al 2023 The Astrophysical Journal 944 .

  • Provider: AAS Journals

Caption: Figure 8.

The net Doppler shifts of Kesseli et al. (2022) (error bars) as compared to this work’s models (crosses). The first phase bin is drawn thinner than the second phase bin; observed phase bins are connected by a dotted line for visibility’s sake. The species are ordered and colored by total observed detection S/N. Rows without crosses correspond to species that we could not recover via cross-correlation in our models. Our models are able to explain some species (e.g., Na), fail to explain others (e.g., Cr) and fail to detect yet others (e.g., K).

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