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Atmospheric Characterization of Six Ultrahot Jupiters from K-band High-resolution Spectroscopy

  • Authors: Luke Finnerty, Michael P. Fitzgerald, Yinzi Xin, Jerry W. Xuan, Julie Inglis, Shubh Agrawal, Ashley Baker, Randall Bartos, Geoffrey A. Blake, Benjamin Calvin, Sylvain Cetre, Jacques-Robert Delorme, Greg Doppmann, Daniel Echeverri, Katelyn Horstman, Chih-Chun Hsu, Nemanja Jovanovic, Joshua Liberman, Ronald A. López, Dimitri Mawet, Evan Morris, Jacklyn Pezzato-Rovner, Jean-Baptiste Ruffio, Ben Sappey, Tobias Schofield, Andrew Skemer, J. Kent Wallace, Nicole L. Wallack, Jason J. Wang, 劲飞 王, Ji Wang, 吉 王

Luke Finnerty et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Orbital phase coverage of our observations, with semimajor axes drawn to scale. The stellar radii are shown as dashed vertical lines in the colors corresponding to each planet to illustrate the start and end of secondary eclipse. We omit portions of the time series for TOI-1518 b, WASP-33 b, WASP-189 b, and KELT-9 b falling within secondary eclipse. WASP-33 b, KELT-9 b, and MASCARA-1 b were observed to significant phase angles.

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