[15.07] SNLS: Relating the properties of type Ia supernovae to the stellar populations of their host galaxies

AAS 207th Meeting, 8-12 January 2006
Session 15 SNLS
Poster, Monday, 9:20am-7:00pm, January 9, 2006, Exhibit Hall

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[15.07] SNLS: Relating the properties of type Ia supernovae to the stellar populations of their host galaxies

M. Sullivan (University of Toronto), C. J. Pritchet (University of Victoria), D. Le Borgne, A. Hodsman, D. A. Howell (University of Toronto), P. Astier (University Paris VI & VII), E. Aubourg (APC, Paris), D. Balam (University of Victoria), S. Basa (LAM, Marseille), R. Carlberg, A. Conley (University of Toronto), S. Fabbro (CENTRA, Lisbon), D. Fouchez (University Aix Marseille II), J. Guy (University Paris VI & VII), I. Hook (University of Oxford), H. Lafoux (DAPNIA, Saclay), J. D. Neill (University of Victoria), R. Pain (University Paris VI & VII), N. Palanque-Delabrouille (DAPNIA, Saclay), K. Perrett (University of Toronto), N. Regnault (University Paris VI & VII), J. Rich (DAPNIA, Saclay), R. Taillet, S. Baumont (University Paris VI & VII), J. Bronder (University of Oxford), M. Filliol (LAM, Marseille), S. Perlmutter (LBL), C. Tao (LAM, Marseille), SNLS Collaboration

We examine the rates and properties of type Ia supernovae (SNe Ia) in relation to the physical parameters defining their host galaxy stellar populations. Using a sample of 114 spectroscopically confirmed SNe Ia discovered via the Supernova Legacy Survey (SNLS) distributed over 0.2

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