Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf

• Main Authors: Baker, A. (Author), Bartos, R. (Author), Blake, G.A (Author), Bond, C.Z (Author), Calvin, B. (Author), Cetre, S. (Author), Delorme, J.-R (Author), Doppmann, G. (Author), Echeverri, D. (Author), Finnerty, L. (Author), Fitzgerald, M.P (Author), Jovanovic, N. (Author), Kent Wallace, J. (Author), Kolecki, J.R (Author), Liu, M.C (Author), Lopez, R. (Author), Mawet, D. (Author), Morris, E. (Author), Pai Asnodkar, A. (Author), Pezzato, J. (Author), Ragland, S. (Author), Roy, A. (Author), Ruane, G. (Author), Ruffio, J.-B (Author), Sappey, B. (Author), Schofield, T. (Author), Skemer, A. (Author), Venenciano, T. (Author), Wallack, N.L (Author), Wang, J. (Author), Wang, J.J (Author), Wizinowich, P. (Author), Xuan, J.W (Author)
• Format: Article
• Language: English
• Published: American Astronomical Society 2022
• Online Access: View Fulltext in Publisher

 A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrievals for substellar objects. Here, we report results of atmospheric retrieval on a synthetic spectrum and a benchmark BD, HR 7672 B, with petitRADTRANS. First, we test the retrieval framework on a synthetic PHOENIX BT-Settl spectrum with a solar composition. We show that the retrieved C and O abundances are consistent with solar values, but the retrieved C/O is overestimated by 0.13-0.18, which is about four times higher than the formal error bar. Second, we perform retrieval on HR 7672 B using high spectral-resolution data (R = 35,000) from the Keck Planet Imager and Characterizer and near-infrared photometry. We retrieve [C/H], [O/H], and C/O to be -0.24 ± 0.05, -0.19 ± 0.04, and 0.52 ± 0.02. These values are consistent with those of HR 7672 A within 1.5σ. As such, HR 7672 B is among only a few benchmark BDs (along with Gl 570 D and HD 3651 B) that have been demonstrated to have consistent elemental abundances with their primary stars. Our work provides a practical procedure of testing and performing atmospheric retrieval, and sheds light on potential systematics of future retrievals using high- and low-resolution data. © 2022. The Author(s). Published by the American Astronomical Society.