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Type IIn Supernovae. I. Uniform Light-curve Characterization and a Bimodality in the Radiated Energy Distribution

  • Authors: Daichi Hiramatsu, Edo Berger, Sebastian Gomez, Peter K. Blanchard, Harsh Kumar, Wasundara Athukoralalage

Daichi Hiramatsu et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 9.

Left: histograms of the r-band timescales (tr) above each 10% flux level relative to peak on the rise and decline. Right: the difference between successive 10% flux levels (Δtr, namely, the inverted slope) on the rise and decline. The vertical lines in each panel mark the median (with its value on the top left) and P15.9P84.1 and P2.3P97.7 ranges. For each distribution, the temporal progression along the light curve is counterclockwise from the left-top to right-top panels. The inverted slope is an increasing function, i.e., the light-curve slope becomes shallower with respect to time.

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