**Table 2:** The test sample of type Ia supernovae light curves.
Name	z ^a	z ^b	Bands	m^*_B ^BV	s ^BV	c ^BV	m^*_B ^UB	s ^UB	c ^UB	Phot. Ref.^c
1990af	0.051	0.050	BV	17.73 $\;$ (0.01)	0.73 $\;$ (0.01)	0.00 $\;$ (0.01)				(H96)
1992bc	0.020	0.020	BVR	15.09 $\;$ (0.01)	1.03 $\;$ (0.01)	-0.04 $\;$ (0.01)				(H96)
1992bh	0.045	0.045	BV	17.60 $\;$ (0.02)	0.97 $\;$ (0.02)	0.10 $\;$ (0.01)				(H96)
1992bo	0.019	0.018	BVR	15.76 $\;$ (0.01)	0.73 $\;$ (0.01)	0.06 $\;$ (0.01)				(H96)
1992bp	0.079	0.079	BV	18.28 $\;$ (0.01)	0.86 $\;$ (0.01)	-0.04 $\;$ (0.01)				(H96)
1993H	0.024	0.025	BVR	16.74 $\;$ (0.02)	0.69 $\;$ (0.01)	0.26 $\;$ (0.02)				(H96, A04)
1993O	0.052	0.053	BV	17.62 $\;$ (0.01)	0.89 $\;$ (0.01)	-0.01 $\;$ (0.01)				(H96)
1993ag	0.049	0.050	BV	17.80 $\;$ (0.01)	0.89 $\;$ (0.02)	0.10 $\;$ (0.02)				(H96)
1995ac	0.050	0.049	BVR	17.04 $\;$ (0.01)	1.03 $\;$ (0.01)	0.01 $\;$ (0.01)				(R99, A04)
1995bd	0.016	0.016	BVR	15.26 $\;$ (0.01)	0.99 $\;$ (0.01)	0.30 $\;$ (0.01)				(R99, A04)
1996bl	0.036	0.035	BVR	16.68 $\;$ (0.01)	0.97 $\;$ (0.01)	0.05 $\;$ (0.01)				(R99)
1996bo	0.017	0.016	UBVR	15.83 $\;$ (0.01)	0.88 $\;$ (0.01)	0.36 $\;$ (0.01)	15.84 $\;$ (0.01)	0.89 $\;$ (0.01)	0.16 $\;$ (0.07)	(R99, A04)
1997E	0.013	0.013	UBVR	15.10 $\;$ (0.01)	0.82 $\;$ (0.01)	0.08 $\;$ (0.01)	15.10 $\;$ (0.01)	0.80 $\;$ (0.01)	0.07 $\;$ (0.02)	(J02)
1998ab	0.027	0.028	UBVR	16.08 $\;$ (0.01)	0.94 $\;$ (0.01)	0.09 $\;$ (0.01)	16.05 $\;$ (0.02)	0.90 $\;$ (0.01)	-0.03 $\;$ (0.02)	(J02)
1999aa	0.014	0.015	UBVR	14.73 $\;$ (0.01)	1.05 $\;$ (0.01)	-0.00 $\;$ (0.01)	14.72 $\;$ (0.01)	1.05 $\;$ (0.01)	-0.00 $\;$ (0.01)	(J02, K00, A00)
1999ac	0.009	0.010	UBVR	14.10 $\;$ (0.01)	0.93 $\;$ (0.01)	0.09 $\;$ (0.01)	14.08 $\;$ (0.01)	0.89 $\;$ (0.02)	0.12 $\;$ (0.02)	(J02)
1999aw	0.038	0.039	BVR	16.75 $\;$ (0.01)	1.19 $\;$ (0.01)	0.04 $\;$ (0.01)				(S02)
1999cc	0.031	0.032	UBVR	16.78 $\;$ (0.01)	0.84 $\;$ (0.01)	0.01 $\;$ (0.01)	16.75 $\;$ (0.02)	0.81 $\;$ (0.02)	0.12 $\;$ (0.03)	(J02)
1999dq	0.014	0.014	UBVR	14.41 $\;$ (0.01)	1.05 $\;$ (0.01)	0.13 $\;$ (0.01)	14.41 $\;$ (0.01)	1.04 $\;$ (0.01)	0.06 $\;$ (0.01)	(J02)
1999ek	0.018	0.018	BVR	15.61 $\;$ (0.01)	0.89 $\;$ (0.01)	0.16 $\;$ (0.01)				(J02, K04b)
1999gp	0.027	0.026	UBVR	16.02 $\;$ (0.01)	1.09 $\;$ (0.01)	0.09 $\;$ (0.01)	16.02 $\;$ (0.01)	1.07 $\;$ (0.01)	0.03 $\;$ (0.01)	(J02, K01)
2000ca	0.024	0.025	UBVR	15.52 $\;$ (0.01)	1.00 $\;$ (0.01)	-0.07 $\;$ (0.01)	15.56 $\;$ (0.01)	0.98 $\;$ (0.02)	-0.05 $\;$ (0.02)	(K04a)
2000cn	0.023	0.023	UBVR	16.55 $\;$ (0.01)	0.73 $\;$ (0.01)	0.19 $\;$ (0.01)	16.56 $\;$ (0.01)	0.73 $\;$ (0.01)	0.18 $\;$ (0.01)	(J02)
2000dk	0.017	0.016	UBVR	15.34 $\;$ (0.01)	0.73 $\;$ (0.01)	0.05 $\;$ (0.01)	15.33 $\;$ (0.01)	0.70 $\;$ (0.01)	0.02 $\;$ (0.01)	(J02)
2001V	0.015	0.016	BVR	14.60 $\;$ (0.02)	1.10 $\;$ (0.02)	0.11 $\;$ (0.02)				(Vi03)
2001ba	0.029	0.031	BV	16.20 $\;$ (0.01)	0.99 $\;$ (0.01)	-0.04 $\;$ (0.01)				(K04a)

^aHeliocentric redshift. ^bCMB-centric redshift. ^cPhotometry references: H96: Hamuy et al. (1996a), R99: Riess et al. (1999), K00: Krisciunas et al. (2000), H01: Howell (2001), L01: Li et al. (2001b), J02: Jha (2002), S02: Strolger et al. (2002), Vi03: Vinkó et al. (2003), Z03: Zapata et al. (2003), A04: Altavilla et al. (2004), G04: Garavini et al. (2004), K04a: Krisciunas et al. (2004), K04b: Krisciunas et al. (2004), G05: Garavini et al. (2005).

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