Image Details
Caption: Figure 7.
The reduced χ2 of the comparison between the reduced GNIRS spectrum of HIP 17453 B and field dwarfs from the IRTF spectral library (M. C. Cushing et al. 2005; J. T. Rayner et al. 2009) and very low/intermediate-gravity objects from the Montreal Spectral Library (J. Gagné et al. 2015), with different classes of objects denoted by the various colors. The spectrum of HIP 17453 B is best fit by the intermediate-gravity early L dwarf objects. A spectral type of L2 ± 1 is adopted as denoted by the gray shaded region.
© 2026. The Author(s). Published by the American Astronomical Society.