Garavini, G., Folatelli, G., Nobili, S., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Blanc, G., Bronder, T., Burns, M.S., Conley, A., Deustua, S.E., Doi, M., Fabbro, S., Fadeyev, V., Gibbons, R., Goldhaber, G., Goobar, A., Groom, D.E., Hook, I., Howell, D.A., Kashikawa, N., Kim, A.G., Kowalski, M., Kuznetsova, N., Lee, B.C., Lidman, C., Mendez, J., Morokuma, T., Motohara, K., Nugent, P.E., Pain, R., Perlmutter, S., Quimby, R., Raux, J., Regnault, N., Ruiz-Lapuente, P., Sainton, G., Schahmaneche, K., Smith, E., Spadafora, A.L., Stanishev, V., Thomas, R.C., Walton, N.A., Wang, L., Wood-Vasey, W.M. and Yasuda, N. (2007), "Quantitative comparison between type Ia supernova spectra at low and high redshifts: a case study", A&A, 470: 411-424.
Abstract: None
Keywords: stars: supernovae: general, cosmology: early Universe
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