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Identifying and Characterizing Very Low-mass Spectral Blend Binaries with Machine Learning Methods

  • Authors: Juan Diego Draxl Giannoni, Malina Desai, Adam J. Burgasser, A. Camille Dunning, Christian Aganze, Luke McDermott, Christopher A. Theissen, Daniella C. Bardalez Gagliuffi

Juan Diego Draxl Giannoni et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 10.

FI for the BClass1 model for low- (top), mid- (middle), and high-S/N (bottom) groups (see Figure 8). Each panel displays FI for primary (magenta) and secondary (blue) classification on linear (middle plot) and logarithmic scales (bottom plot), compared to an L5 plus T5 synthetic binary spectrum with an S/N in the associated range (top plot). Regions associated with telluric (gray), K I (green), CH4 (blue), and CO (red) absorption are indicated by vertical bands.

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