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Asymmetric Nightside CO2 Features, Inefficient Heat Transport, and Precise Evolutionary Constraints: Spectroscopic Phase Curves Reveal the Past and Present of a White Dwarf–Brown Dwarf Binary

  • Authors: Daphne Broski-Laing, Yifan Zhou, Joshua D. Lothringer, Daniel Apai, Jenni R. French, Sarah L. Casewell, L. C. Mayorga, Lael Shin, Ben W. P. Lew, Xianyu Tan, Vivien Parmentier, Siyi Xu, Mark S. Marley

Daphne Broski-Laing et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

Best-fit batman transit model of ZTF0038 fit via Markov Chain Monte Carlo using emcee. The brown dwarf’s emission is subtracted, and the flux is normalized such that the out-of-eclipse signal is centered around 1 and the flux reaches zero during the total eclipse.

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