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J. A. Cardelli, G. .C. Clayton, J. .S. Mathis, ApJ
1989
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S. Jha, A. G. Riess, R. P. Kirshner, ApJ
2007
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2007
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2009

Dark Energy Survey Supernovae: Simulations and Survey Strategy

Bernstein, J. P., Kessler, R., Kuhlmann, S. et al.

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We present simulations for the Dark Energy Survey (DES) using a new code suite (SNANA) that generates realistic supernova light curves accounting for atmospheric seeing conditions and intrinsic supernova luminosity variations using MLCS2k2 or SALT2 models.

Errors include stat-noise from photo-statistics and sky noise.
We applied SNANA to simulate DES supernova observations and employed an MLCS-based fitter to obtain the distance modulus for each simulated light curve.
We harnessed the light curves in order to study selection biases for high-redshift supernovae and to constrain the optimal DES observing strategy using the Dark Energy Task Force figure of merit.