Figure 8.
Top panel: I-band absolute magnitude on day 50 versus plateau duration. The plateau length stays approximately constant over a large range of magnitudes, though perhaps getting shorter for brighter SNe. Bottom panel: photospheric velocities on day 50 versus plateau duration. Since there is an established correlation between luminosity and velocity for SNe II-P, the plot resembles the one in the top panel. The red dots are a subset of grid models computed by Dessart et al. (2010), interpolated to satisfy the mass–velocity relation found by Poznanski (2013). These models show very good agreement with our measurements.

Top panel: I-band absolute magnitude on day 50 versus plateau duration. The plateau length stays approximately constant over a large range of magnitudes, though perhaps getting shorter for brighter SNe. Bottom panel: photospheric velocities on day 50 versus plateau duration. Since there is an established correlation between luminosity and velocity for SNe II-P, the plot resembles the one in the top panel. The red dots are a subset of grid models computed by Dessart et al. (2010), interpolated to satisfy the mass–velocity relation found by Poznanski (2013). These models show very good agreement with our measurements.

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