In the past three years two separate programs were initiated to study the restframe UV properties of Type Ia Supernovae. 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
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
Large photometric surveys with the aim of identifying many Type Ia supernovae (SNe) at moderate reds...
We analyze the mean rest-frame ultraviolet (UV) spectrum ofType Ia Supernovae(SNe) and its dispersio...
In the past three years two separate programs were initiated to study the restframe UV properties o...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae(SNe) and its dispers...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe Ia) and its disp...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
We present an analysis of the maximum light, near-ultraviolet (NUV; 2900 < λ < 5500̴...
We present spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by...
We present spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by...
We present the first results of an ongoing campaign using the STIS spectrograph on board the Hubble ...
To extract useful cosmological information from type Ia supernovae (SNe Ia), standardization laws ha...
Accepted for publication in AJ. Also available at http://supernova.lbl.gov/We present spectra for 14...
We present an analysis of the maximum light, near ultraviolet (NUV; 2900-5500 A) spectra of 32 low r...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
Large photometric surveys with the aim of identifying many Type Ia supernovae (SNe) at moderate reds...
We analyze the mean rest-frame ultraviolet (UV) spectrum ofType Ia Supernovae(SNe) and its dispersio...
In the past three years two separate programs were initiated to study the restframe UV properties o...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae(SNe) and its dispers...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe Ia) and its disp...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
We present an analysis of the maximum light, near-ultraviolet (NUV; 2900 < λ < 5500̴...
We present spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by...
We present spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by...
We present the first results of an ongoing campaign using the STIS spectrograph on board the Hubble ...
To extract useful cosmological information from type Ia supernovae (SNe Ia), standardization laws ha...
Accepted for publication in AJ. Also available at http://supernova.lbl.gov/We present spectra for 14...
We present an analysis of the maximum light, near ultraviolet (NUV; 2900-5500 A) spectra of 32 low r...
We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispers...
Large photometric surveys with the aim of identifying many Type Ia supernovae (SNe) at moderate reds...
We analyze the mean rest-frame ultraviolet (UV) spectrum ofType Ia Supernovae(SNe) and its dispersio...