NIRSpec/prism spectra of the seven RUBIES brown dwarfs identified in this study (black lines). Spectra are shown in apparent F_λ flux densities after scaling to their F444W magnitudes, and uncertainties are indicated in gray. Key spectral features present in the 1–5 μm spectra of L and T dwarfs are labeled.

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)