Fig. 12

SN Iaα corrected Hubble residual distributions
(, blue-filled histogram),
and its best Gaussian fit (solid-blue line, one 3σ-outlier
rejected). The standardization has been performed on only SNe Iaα.
For comparison, the full sample residual distribution (for a full sample
standardization) is shown by the open histogram, with its best Gaussian fit in gray.
Both distributions where generated from independent standardizations and are
therefore centered on zero.
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