J. P. Bernstein, R. Kessler, S. Kuhlmann, R. Biswas, E. Kovacs, G. Aldering, I. Crane, D. A. Finley, J. A. Frieman, T. Hufford, M. J. Jarvis, A. G. Kim, J. Marriner, P. Mukherjee, R. C. Nichol, P. Nugent, D. Parkinson, R. R. R. Reis, M. Sako, H. Spinka, M. Sullivan
We present an analysis of supernova light curves simulated for the upcoming
Dark Energy Survey (DES) supernova search. The simulations employ a code suite
that generates and fits realistic light curves in order to obtain distance
modulus/redshift pairs that are passed to a cosmology fitter. We investigated
several different survey strategies including field selection, supernova
selection biases, and photometric redshift measurements. Using the results of
this study, we chose a 30 square degree search area in the griz filter set. We
forecast 1) that this survey will provide a homogeneous sample of up to 4000
Type Ia supernovae in the redshift range 0.05View original: http://arxiv.org/abs/1111.1969
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