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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 1.

Left: outline of the custom spectral extraction pipeline used to generate absolute-flux-calibrated time-series spectra. Right: intermediate data products generated at various stages throughout the reduction process: (A) relative flux-calibrated spectral time series produced by Eureka!; (B) flux-calibrated and exposure-averaged spectra produced by the jwst pipeline; (C) master calibration factor array; and (D) absolute-flux-calibrated spectral time series. These time-series spectra include a few visible outlier integrations, which are noted in Table 1 and excluded from all subsequent analysis.

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