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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Egile Nagusiak:	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
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	Institute of Physics Publishing 2008

SiFTO: An empirical method for fitting SN Ia light curves nork 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

Argitaratua 2008

Journal article

SiFTO: An empirical method for fitting SN Ia light curves

SiFTO: An empirical method for fitting SN Ia light curves nork 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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