A Type II Supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS Surveys
The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct...
Guardado en:
| Autores principales: | Jaeger, T. de, González Gaitán, S., Hamuy, M., Galbany, L., Anderson, J. P., Phillips, M. M., Stritzinger, M. D., Carlberg, R. G., Sullivan, M., Gutiérrez, C. P., Hook, I. M., Howell, D. A., Hsiao, E. Y., Kuncarayakti, H., Ruhlmann Kleider, V., Folatelli, Gastón, Pritchet, C., Basa, S. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/87279 |
| Aporte de: |
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