- Bailey, S;
- Aldering, G;
- Antilogus, P;
- Aragon, C;
- Baltay, C;
- Bongard, S;
- Buton, C;
- Childress, M;
- Copin, Y;
- Gangler, E;
- Loken, S;
- Nugent, P;
- Pain, R;
- Pecontal, E;
- Pereira, R;
- Perlmutter, S;
- Rabinowitz, D;
- Rigaudier, G;
- Ripoche, P;
- Runge, K;
- Scalzo, R;
- Smadja, G;
- Tao, C;
- Thomas, RC;
- Wu, C
The use of Type Ia supernovae as distance indicators led to the discovery of
the accelerating expansion of the universe a decade ago. Now that large second
generation surveys have significantly increased the size and quality of the
high-redshift sample, the cosmological constraints are limited by the currently
available sample of ~50 cosmologically useful nearby supernovae. The Nearby
Supernova Factory addresses this problem by discovering nearby supernovae and
observing their spectrophotometric time development. Our data sample includes
over 2400 spectra from spectral timeseries of 185 supernovae. This talk
presents results from a portion of this sample including a Hubble diagram
(relative distance vs. redshift) and a description of some analyses using this
rich dataset.