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N.V. Kuznetsova (Lawrence Berkeley Lab), A. Bonissent (Centre de Physique des Particules de Marseille), A.G. Kim (Lawrence Berkeley Lab)
We study the performance of the SNAP simulation lightcurve fitter. The errors on the parameters extracted by the fitter are examined as a function of signal to noise, for various observing cadences, and for different epochs in the type Ia supernova lifetime.
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.