Ultraviolet Spectroscopy of Type Ia Supernovae at Low- and High-Redshift

Details Ultraviolet Spectroscopy of Type Ia Supernovae at Low- and High-Redshift Ultraviolet Spectroscopy of Type Ia Supernovae at Low- and High-Redshift

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..342..224n&link_type=abstract

1604-2004: Supernovae as Cosmological Lighthouses, ASP Conference Series, Vol. 342, Proceedings of the conference held 15-19 Jun

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In the past three years two separate programs were initiated to study the restframe UV properties of Type Ia Supernovae (SNe). The low-redshift study was carried out using several ground-based facilities coupled with HST/STIS observations. The high-redshift program is an offshoot of the CFHT Legacy Survey and uses Keck/LRIS to obtain spectra. Here we present the preliminary results from each program and their implications for current cosmology measurements.

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