Gamma-ray bursts with wider prompt-emission spectra tend to be longer, brighter, and more energetic, though the rest-frame correlation becomes significant only after removing outliers.
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A Connection between Spectral Width and Energetics As Well As Peak Luminosity in Fermi Gamma-Ray Bursts
Gamma-ray bursts with wider prompt-emission spectra tend to be longer, brighter, and more energetic, though the rest-frame correlation becomes significant only after removing outliers.