Authors:
Patat, F
Cappellaro, E
Danziger, J
Mazzali, PA
Sollerman, J
Augusteijn, T
Brewer, J
Doublier, V
Gonzalez, JF
Hainaut, O
Lidman, C
Leibundgut, B
Nomoto, K
Nakamura, T
Spyromilio, J
Rizzi, L
Turatto, M
Walsh, J
Galama, TJ
van Paradijs, J
Kouveliotou, C
Vreeswijk, PM
Frontera, F
Masetti, N
Palazzi, E
Pian, E
Citation: F. Patat et al., The metamorphosis of SN 1998bw, ASTROPHYS J, 555(2), 2001, pp. 900-917
Authors:
Nakamura, T
Mazzali, PA
Nomoto, K
Iwamoto, K
Citation: T. Nakamura et al., Light curve and spectral models for the hypernova sn 1998bw associated with GRB 980425, ASTROPHYS J, 550(2), 2001, pp. 991-999
Authors:
Mazzali, PA
Nomoto, K
Cappellaro, E
Nakamura, T
Umeda, H
Iwamoto, K
Citation: Pa. Mazzali et al., Can differences in the nickel abundance in chandrasekhar-mass models explain the relation between the brightness and decline rate of normal type Ia supernovae?, ASTROPHYS J, 547(2), 2001, pp. 988-994
Citation: Pa. Mazzali, Applications of an improved Monte Carlo code to the synthesis of early-time Supernova spectra, ASTRON ASTR, 363(2), 2000, pp. 705-716
Authors:
Nakamura, T
Mazzali, PA
Nomoto, K
Iwamoto, K
Umeda, H
Citation: T. Nakamura et al., A 'hypernova' model for the supernova 1998bw possibly associated with GRB980425, ASTRON NACH, 320(4-5), 1999, pp. 363-363