TRAPPIST-1 flares follow a single power law N(≥E_TESS) ∝ E_TESS^{-0.753} from 10^{29} to 10^{33} erg after sensitivity corrections and bandpass conversion.
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Proposes the Nautilus observatory concept for time-resolved flare spectroscopy on GKM stars to create empirical spectral templates for improved planetary habitability simulations.
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A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy
TRAPPIST-1 flares follow a single power law N(≥E_TESS) ∝ E_TESS^{-0.753} from 10^{29} to 10^{33} erg after sensitivity corrections and bandpass conversion.
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Nautilus: Fast Time-Resolved Spectroscopy of GKM Stellar Flares and Their Implications for Planetary Habitability
Proposes the Nautilus observatory concept for time-resolved flare spectroscopy on GKM stars to create empirical spectral templates for improved planetary habitability simulations.