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A White-light Flare on the L1 Dwarf WISEP J190648.47+401106.8

  • Authors: Ashton Southwick, Easton J. Honaker, John E. Gizis, Riley W. Clarke, Tyler Blask, Harrison Petrie

Ashton Southwick et al 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

Caption: Figure 1.

Top: χ2 parameter space illustrating the covariance between flare temperature and filling factor (﹩{X}_{{\rm{flare}}}﹩). A white dot represents the best-fit with T = 12,850 ± 25 K and a filling factor of 4.45 × 10−4. Bottom: the observed flaring spectrum (red) and non-flare spectrum (gray). The best-fit spectrum (blue) was calculated using data λ < 750 nm, with Hα and other atmospheric features masked during the fit.

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