SiFTO: An empirical method for fitting SN Ia light curves

We present SiFTO, a new empirical method for modeling Type Ia supernova (SN Ia) light curves by manipulating a spectral template. We make use of high-redshift SN data when training the model, allowing us to extend it bluer than rest-frame U. This increases the utility of our high-redshift SN observa...

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Autors principals:	Conley, A, Sullivan, M, Hsiao, E, Guy, J, Astier, P, Balam, D, Balland, C, Basa, S, Carlberg, R, Fouchez, D, Hardin, D, Howell, D, Hook, I, Pain, R, Perrett, K, Pritchet, C, Regnault, N
Format:	Journal article
Idioma:	English
Publicat:	Institute of Physics Publishing 2008

SiFTO: An empirical method for fitting SN Ia light curves per Conley, A, Sullivan, M, Hsiao, E, Guy, J, Astier, P, Balam, D, Balland, C, Basa, S, Carlberg, R, Fouchez, D, Hardin, D, Howell, D, Hook, I, Pain, R, Perrett, K, Pritchet, C, Regnault, N

Publicat 2008

Journal article

SiFTO: An empirical method for fitting SN Ia light curves

SiFTO: An empirical method for fitting SN Ia light curves per Conley, A, Sullivan, M, Hsiao, E, Guy, J, Astier, P, Balam, D, Balland, C, Basa, S, Carlberg, R, Fouchez, D, Hardin, D, Howell, D, Hook, I, Pain, R, Perrett, K, Pritchet, C, Regnault, N

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