Table 2: Fitting results for the light curves of SN 2006aj attained by either excluding early data (top) or including an additional power-law component decaying with index $\alpha$ (see text for details).
$\chi^2_\nu$ k s $\alpha$

B 1.83 $0.734\pm0.014$ $0.620\pm0.006$ $\cdots$

V 1.02 $0.724\pm0.007$ $0.682\pm0.005$ $\cdots$

R 1.93 $0.735\pm0.007$ $0.689\pm0.006$ $\cdots$

I 0.71 $0.761\pm0.008$ $0.686\pm0.008$ $\cdots$

B 1.79 $0.721\pm0.022$ $0.613\pm0.005$ $1.53\pm0.43$

V 0.35 $0.640\pm0.014$ $0.659\pm0.008$ $0.40\pm0.09$

R 0.94 $0.621\pm0.022$ $0.656\pm0.012$ $0.12\pm0.10$

I 0.48 $0.667\pm0.039$ $0.663\pm0.022$ $-0.10\pm0.34$

**Table 2:** Fitting results for the light curves of SN 2006aj attained by either excluding early data (top) or including an additional power-law component decaying with index $\alpha$ (see text for details).
	$\chi^2_\nu$	k	s	$\alpha$
B	1.83	$0.734\pm0.014$	$0.620\pm0.006$	$\cdots$
V	1.02	$0.724\pm0.007$	$0.682\pm0.005$	$\cdots$
R	1.93	$0.735\pm0.007$	$0.689\pm0.006$	$\cdots$
I	0.71	$0.761\pm0.008$	$0.686\pm0.008$	$\cdots$
B	1.79	$0.721\pm0.022$	$0.613\pm0.005$	$1.53\pm0.43$
V	0.35	$0.640\pm0.014$	$0.659\pm0.008$	$0.40\pm0.09$
R	0.94	$0.621\pm0.022$	$0.656\pm0.012$	$0.12\pm0.10$
I	0.48	$0.667\pm0.039$	$0.663\pm0.022$	$-0.10\pm0.34$

Source LaTeX | All tables | In the text