Image Details
Caption: Figure 9.
Comparison between the HIP 17453 B GNIRS spectrum and the BT-Settl (left) and Sonora Diamondback (right) model grids using splat(A. J. Burgasser & Splat Development Team 2017). The best-fitting temperatures and surface gravities range between Teff = 1600–2000 K and log(g) = 5.0–5.5. The Sonora Diamondback fits prefer cloudy models.
© 2026. The Author(s). Published by the American Astronomical Society.