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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 7.

Peak magnitudecolor evolution relation. Absolute peak magnitudes in the 400 nm band, M(400), vs. the color change from peak to +30 days (rest frame). We define ΔM(400–520)30 = (M0(400)–M0(520)) − (M30(400)–M30(520)). The bands at 400 nm and 520 nm are defined in Section 3.2, and the values for ΔM(400–520)30 are reported in Table 1. Left: a plot of eight of the pure sample that have the necessary bands covered in the observer frame to calculate this color term. Right: 11 objects of the complete sample that have the necessary data. The black lines are least-squares straight-line fits to all data in each plot. The red dotted line leaves out CSS121015. The parameters of these line fits are listed in Table 3.

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