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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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