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The JWST/NIRISS Deep Spectroscopic Survey for Young Brown Dwarfs and Free-floating Planets

  • Authors: Adam B. Langeveld, Aleks Scholz, Koraljka Mužić, Ray Jayawardhana, Daniel Capela, Loïc Albert, René Doyon, Laura Flagg, Matthew de Furio, Doug Johnstone, David Lafrèniere, Michael Meyer

Adam B. Langeveld et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 6.

Comparison of the spectral type (left) and extinction A J (right) determined with our template fitting, with the average spectral type given in K. L. Luhman et al. (2016). Spectral types are coded as a linear scale, M5 is 5.0 and L2 is 12.0. The orange line marks the 1:1 relation, the shaded region corresponds to errors of 1 spectral subtype and 1 mag in J-band extinction. For two objects (blue points), we show two possible solutions (joined with dotted–dashed lines); based on magnitudes and colors, the solution with late-M spectral type is preferred.

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