SNLS: Supernova Rise Times from the SNLS Sample

Autor: Conley, A., Howell, D. A., Howes, A., Astier, P., Aubourg, E., Balam, D., Basa, S., Carlberg, R. G., Fabbro, S., Fouchez, D., Guy, J., Hook, I., Lafoux, H., Neill, J. D., Pain, R., Palanque-Delabrouille, N., Perett, K., Pritchet, C. J., Regnault, N., Rich, J., Sullivan, M., Taillet, Richard, Baumont, S., Bronder, J., Lusset, V., Ripoche, P., Mourao, A., Perlmutter, S., Tao, C.

Publikováno v: Bulletin of the American Astronomical Society
American Astronomical Society Meeting 207
American Astronomical Society Meeting 207, Jan 2006, Washington, DC, United States. pp.1176

International audience; Type Ia supernovae (SNe Ia) provide the most direct evidence for the acceleration of the Universe. This evidence relies on a comparison between the luminosities of distant and nearby SNe Ia, and hence is potentially sensitive

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::678e780e87a08e6a9ef24192ab845459
http://hal.in2p3.fr/in2p3-00186302