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Superluminous Supernovae as Standardizable Candles and High-redshift Distance Probes

  • Authors: C. Inserra and S. J. Smartt

Inserra & Smartt 2014 The Astrophysical Journal 796 87.

  • Provider: AAS Journals

Caption: Figure 5.

Peak magnitudedecline rate relation. The absolute peak magnitude in the 400 nm band, M(400), is plotted vs. ΔM10(400), ΔM20(400), and ΔM30(400). The latter three values are measures of the light curve decline (in magnitudes) during the first 10, 20, and 30 days after maximum. The left-hand column of plots shows only the 2005ap-like events (pure sample), and the right-hand column shows all SLSN. The dashed red line is the fit of the extended sample, and the black of the complete sample (see Section 2 for the sample definitions). The SNe magnitudes and the corresponding ΔMday(400) are reported in Table 1, and the parameters of the linear regression fits (black line) are listed in Table 3.

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