**Table 5:** Main parameters of the SNe sample.
SN	SN	Host	Distance	$A_{\rm V}$	$\gamma_V$ $^\ddag$	Max-to-tail contrast	References
name	type	galaxy	(Mpc)	(mag)	(mag (100 d)^-1)	(mag)
1990I	Ib	NGC 4650	39.3 $^\star$	0.4	$\sim$ 5.7	$\sim$ 1.05	this work
1983I	Ic	NGC 4051	13.17 $^\star$	0.043	$\sim$ 8.4	$\sim$ 2.2	1, 2
1984L	Ib	NGC 0991	20.44 $^\star$	0.0	-	-	3, 4, 5
1987M	Ic	NGC 2715	22.7 $^\star$	1.3	-	-	6
1991D	Ib	PGC 84044	178.52 $^\star$	0.186	-	-	7
1993J	IIb	M81	3.64	0.93	$\sim$ 7	$\sim$ 1.23	8
1994I	Ic	NGC 5194	8.32	1.4	$\sim$ 11	$\sim$ 2.42	9
1996N	Ib	NGC 1398	22	0.0	-	-	10
1998bw	Ic-Hypernova	ESO 184-G82	35.16 $^\star$	0.2	$\sim$ 6	$\sim$ 1.64	11, 12, 13, 14

Refs.: 1- Tsvetkov (1985); 2- Tsvetkov (1988); 3- Meikle et al. (1984); 4- Buta (1984); 5- Tsvetkov (1987); 6- Filippenko et al. (1990); 7- Benetti et al. (2002); 8- Lewis et al. (1994); 9- Richmond et al. (1996); 10- Sollerman et al. (1998); 11- Galama et al. (1998); 12- McKenzie & Schaefer (1999); 13- Patat et al. (2001); 14- Sollerman et al. (2000).
$^\star$ Estimated using "LEDA'' database and adopting $H_0=70~ {\rm km ~s^{-1} Mpc^{-1}}$ .
$^\ddag$ Early decline rate from maximum.

Source LaTeX | All tables | In the text