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Table 3

Maximum likelihood parameter estimates (μ,σ,ξ) obtained from the distance modulus Monte-Carlo with different light-curve fitters (cf. Fig. 6).

Fitter μ σ ξ 1-CDF

MLCS2k2(1.7) 2.11 0.47 –0.10 5.1%
MLCS2k2(3.1) 2.14 0.48 –0.12 4.4%
SALT 2.40 0.56 –0.11 86.2%
SALT II 2.47 0.55 –0.11 30.3%

Notes.The last column contains the probability of measuring higher Hubble asymmetries than the original ones according to the fitted distribution.

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