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A High-resolution Spectroscopic Survey of Directly Imaged Companion Hosts. III. Characterization of the Cold Imaged Planet Hosts AF Lep A and ϵ Indi A

  • Authors: Aneesh Baburaj, Quinn M. Konopacky, Christopher A. Theissen, Jerry W. Xuan, Roman Gerasimov, Kielan K. W. Hoch

Aneesh Baburaj et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 2.

Posteriors for MARCS–C/S grid fit to spectral order #51 with the S I feature at 6757 Å. The marginalized posteriors are shown along the diagonal. The blue lines represent the 50 percentile, and the dotted lines represent the 16 and 84 percentiles. The subsequent covariances between all the parameters are in the corresponding 2D histograms. We obtain a best-fit ﹩\mathrm{log}{\epsilon }_{S}﹩ = 7.12 ± 0.03. Note that the latter uncertainty values solely represent the fitting uncertainties. Other parameters (including carbon abundance) are not well-constrained fitting this order.

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