Spectroscopy of Type Ia supernovae (Bronder+, 2008)

Computer Science

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Supernovae, Photometry, Equivalent Widths

Scientific paper

Full details of the methods used for CFHT Supernova Legacy Survey (SNLS) SN candidate selection and observation can be found in Sullivan et al. (2006AJ....131..960S) and Howell et al. (2005ApJ...634.1190H), respectively. In summary, the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS), using the Megacam wide field imager, acquires real time light-curves of possible SNe by repeatedly imaging four, one square-degree fields approximately every four days (observers' frame) in several filters (a combination of g', r', i', and z') as part of the Deep component of the CFHTLS. Spectroscopic observations are then made at 8m-class telescopes in order to identify the SN-type and redshift of these candidates.
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