| Autor: |
Bronder, T. J., Hook, I. M., Astier, P., Balam, D., Balland, C., Basa, S., Carlberg, R. G., Conley, A., Fouchez, D., Guy, J., Howell, D. A., Neill, J. D., Pain, R., Perrett, K., Pritchet, C. J., Regnault, N., Sullivan, M., Baumont, S., Fabbro, S., Filliol, M., Perlmutter, S., Ripoche, P., Bronder, T. J., Hook, I. M., Astier, P., Balam, D., Balland, C., Basa, S., Carlberg, R. G., Conley, A., Fouchez, D., Guy, J., Howell, D. A., Neill, J. D., Pain, R., Perrett, K., Pritchet, C. J., Regnault, N., Sullivan, M., Baumont, S., Fabbro, S., Filliol, M., Perlmutter, S., Ripoche, P. |
| Zdroj: |
Astronomy and Astrophysics; January 2008, Vol. 477 Issue: 3 p717-734, 18p |
| Abstrakt: |
Aims.We present a quantitative study of a new data set of high redshift Type Ia supernovae spectra, observed at the Gemini telescopes during the first 34 months of the Supernova Legacy Survey. During this time 123 supernovae candidates were observed, of which 87 have been identified as SNe Ia at a median redshift of $z=0.720$. Spectra from the entire second year of the survey and part of the third year (59 total SNe candidates with 46 confirmed SNe Ia) are published here for the first time. The spectroscopic measurements made on this data set are used determine if these distant SNe comprise a population similar to those observed locally. |
| Databáze: |
Supplemental Index |
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