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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 4.

Histograms of the raw (uncorrected) absolute peak magnitudes, M(400), for the three samples defined in Section 2. The dashed lines are least-squares, best-fit Gaussians. Assuming confidence limits for a small number of events from Gehrels (1986), the Gaussian fits all comfortably fall within the 1σ errors of the frequencies.

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