Online Material

 

Table 1: The position angle and inclination of the disk

Galaxy i		i/PA	i/PA	i
		method 1	method 2	litt(25)
Arp 70	A	51 $\pm$ 3	48/158 (24)	74/150
	B	58 $\pm$ 2	59/146 (25)
Arp 74	A	20 $\pm$ 10	17/63? (26)	17/-
	B	46 $\pm$ 5	44/6 (26)
Kar 64	A	51 $\pm$ 2	53/47 (25)	50/50
Kar 64	B	70 $\pm$ 3	68/90 (25)	79/93
Kar 125	A	< 20	17/131 (25)	17/136
Kar 125	B	51 $\pm$ 2	49/53 (26)	21/126
Arp 82	A	51 $\pm$ 5	51/0* (26)	63/-
	B		56/60 (26)	46/112
Kar 168	A	74 $\pm$ 2	71/141 (26)	74/148
Kar 168	B	80 $\pm$ 5	75/102 (26)
Kar 179	A	< 41	31/156 (26)	32/69
Kar 179	B	74 $\pm$ 3	70/164 (26)	68/165
Kar 203	A	< 46	38/125 (26)	57/145
Kar 203	B	51 $\pm$ 5	48/20 (26)	54/13
Kar 296	A		54/127 (24)	52/-
Kar 296	B	74 $\pm$ 3	78/59 (24)	75/52
Arp 87	A	46 $\pm$ 5	57/111 (25)	59/123
	B	62 $\pm$ 5	51/63 (25)	68/-
Kar 302	A	51 $\pm$ 2	41/170 (26)	54/165
Kar 302	B	46 $\pm$ 3	57/114 (26)	46/125
Kar 331	A	51 $\pm$ 3	46/27 (25)	51/15
Kar 331	B	65 $\pm$ 3	59/169 (25)
Arp 183		51 $\pm$ 3	60/88 (26)	21/-
Arp 36		62 $\pm$ 5	61/12 (25)	65/12
Kar 404	A	51 $\pm$ 5	55/18 (26)	58/-
Kar 404	B	62 $\pm$ 3	59/174 (26)	59/167
NGC 5905			50/125 (26)	50/135
NGC 5908		<60	76/156 (26)	71/154
Kar 471	A		41/168 (26)	38/130
Kar 471	B	35 $\pm$ 5	43/72 (26)	43/140
Arp 218	A	50 $\pm$ 5	60/35* (25)	60/-
Arp 218	B	70 $\pm$ 5	62/48 (25)
Kar 523	A	40 $\pm$ 3	41/38 (25)
Kar 523	B	40 $\pm$ 5	37/148 (24)	60/145
Kar 538	A		27/55* (25)	35/-
Kar 538	B		42/35 (25)	47/-
Arp 298	A	40 $\pm$ 3	48/120 (25)	45/125
Arp 298	B	50 $\pm$ 3	58/116 (25)	63/54

* Values are very uncertain.

All inclinations have been corrected by the Hubble formula as explained in the text. Method 1 and 2 are explained in the text. The literature values are measured at the surface brightness level of 25 mag arcsec^-2 (RC3). The values in parenthesis indicate the surface brightness levels used in the measurements.

 

Table 2: The effective and integrated parameters of the profiles

Galaxy	Filt	R25	m25	$r_{\rm e}$	$\mu_{\rm e}$	m	MB(corr)
Arp 70A	B	22.7 $\pm$ 3.0	15.24 $\pm$ 0.17	13.6 $\pm$ 0.1	23.40 $\pm$0.04	14.81 $\pm$ 0.17(27.2)	-20.94
	V	33.2 $\pm$ 1.0	14.16 $\pm$ 0.06	11.5 $\pm$ 0.1	22.24 $\pm$ 0.02	13.95 $\pm$ 0.06(26.1)
	R	42.8 $\pm$ 2.8	13.45 $\pm$ 0.05	9.9 $\pm$ 0.1	21.43 $\pm$ 0.01	13.36 $\pm$ 0.05(25.8)
	I	56.1 $\pm$ 2.8	12.86 $\pm$ 0.08	9.8 $\pm$ 0.1	21.01 $\pm$0.01	12.86 $\pm$ 0.08(25.2)
Arp 70B	B	11.6 $\pm$ 0.7	16.42 $\pm$ 0.18	6.0 $\pm$ 0.2	23.21 $\pm$ 0.04	16.00 $\pm$ 0.18(26.4)	-19.75
	V	16.4 $\pm$ 1.4	15.30 $\pm$ 0.07	4.7 $\pm$ 0.1	21.74 $\pm$ 0.01	15.09 $\pm$ 0.07(26.0)
	R	19.7 $\pm$ 1.3	14.65 $\pm$ 0.06	4.4 $\pm$ 0.1	20.91 $\pm$ 0.00	14.52 $\pm$ 0.06(25.8)
	I	26.5 $\pm$ 2.0	14.10 $\pm$ 0.09	4.6 $\pm$ 0.1	20.44 $\pm$ 0.00	14.04 $\pm$ 0.09(25.4)
Arp 74A	B	35.0 $\pm$ 0.6	14.97 $\pm$ 0.19	25.8 $\pm$ 0.2	24.42 $\pm$ 0.11	14.51 $\pm$ 0.24	-19.86
	V	45.9 $\pm$ 0.8	13.82 $\pm$ 0.06	23.0 $\pm$ 0.6	23.31 $\pm$ 0.04	13.64 $\pm$ 0.13
	R	50.1 $\pm$ 0.3	13.24 $\pm$ 0.06	21.1 $\pm$ 0.1	22.65 $\pm$ 0.02	13.17 $\pm$ 0.08
	I	53.8 $\pm$ 1.8	12.68 $\pm$ 0.04	22.0 $\pm$ 0.7	22.15 $\pm$ 0.03	12.58 $\pm$ 0.14
Arp 74B	B	11.5 $\pm$ 0.8	17.20 $\pm$ 0.21	8.5 $\pm$ 0.1	24.32 $\pm$ 0.11	16.68 $\pm$ 0.25	-17.69
	V	16.7 $\pm$ 0.6	15.95 $\pm$ 0.09	7.7 $\pm$ 0.1	23.06 $\pm$ 0.03	15.70 $\pm$ 0.22
	R	19.6 $\pm$ 0.4	15.36 $\pm$ 0.08	7.4 $\pm$ 0.1	22.49 $\pm$ 0.02	15.20 $\pm$ 0.20
	I	26.3 $\pm$ 0.9	14.65 $\pm$ 0.11	8.5 $\pm$ 0.1	22.26 $\pm$ 0.02	14.53 $\pm$ 0.20
Kar 64A	B	69.0 $\pm$ 0.7*	13.69 $\pm$ 0.22*
	V	71.0 $\pm$ 4.0	12.63 $\pm$ 0.06	32.0 $\pm$ 0.3	22.83 $\pm$ 0.07	12.54 $\pm$ 0.03
	R	72.6 $\pm$ 3.2	12.28 $\pm$ 0.05	30.7 $\pm$ 0.9	22.47 $\pm$ 0.05	12.20 $\pm$ 0.20
	I	76.8 $\pm$ 0.6	11.99 $\pm$ 0.07	27.8 $\pm$ 0.3	22.08 $\pm$ 0.01	11.94 $\pm$ 0.19
Kar 64B	B	28.4 $\pm$ 1.6	15.34 $\pm$ 0.17	19.2 $\pm$ 0.4	24.00 $\pm$ 0.04	14.99 $\pm$ 0.17(26.2)	-19.99
	V	36.2 $\pm$ 2.3	14.07 $\pm$ 0.06	21.4 $\pm$ 0.6	23.24 $\pm$ 0.06	13.64 $\pm$ 0.06(26.4)
	R	44.8 $\pm$ 3.5	13.60 $\pm$ 0.05	24.3 $\pm$ 0.6	23.21 $\pm$ 0.05	13.15 $\pm$ 0.05(25.7)
	I	53.8 $\pm$ 2.6	13.18 $\pm$ 0.07	23.7 $\pm$ 0.3	22.88 $\pm$0.03	12.83 $\pm$ 0.07(25.4)
Kar 125A	B	33.7 $\pm$ 2.6	13.55 $\pm$ 0.14	8.2 $\pm$ 0.2	21.12 $\pm$ 0.02	13.42 $\pm$ 0.16	-20.82
	V	42.7 $\pm$ 3.6*	12.77 $\pm$ 0.07*	8.4 $\pm$ 0.2	20.44 $\pm$ 0.03	12.75 $\pm$ 0.07
	R	43.6 $\pm$ 2.2*	12.24 $\pm$ 0.06*	8.0 $\pm$ 0.2	19.75 $\pm$ 0.02	12.22 $\pm$ 0.07
	I	49.5 $\pm$ 1.8*	11.69 $\pm$ 0.09*	8.4 $\pm$ 0.2	19.37 $\pm$ 0.01	11.60 $\pm$ 0.10
Kar 125B	B	45.0 $\pm$ 0.6*	12.97 $\pm$ 0.05*
Arp 82A	B	54.9 $\pm$ 0.9	13.62 $\pm$ 0.01	33.6 $\pm$ 0.3	23.53 $\pm$ 0.02	13.30 $\pm$ 0.01(26.7)	-20.40
	V	64.8 $\pm$ 0.9	12.87 $\pm$ 0.01	32.4 $\pm$ 0.3	23.00 $\pm$ 0.01	12.69 $\pm$ 0.01(26.3)
	R	70.5 $\pm$ 2.1	12.37 $\pm$ 0.01	32.0 $\pm$ 0.8	22.45 $\pm$ 0.02	12.20 $\pm$ 0.01(25.7)
	I	108.0 $\pm$ 1.5	11.48 $\pm$ 0.01	34.9 $\pm$ 0.3	21.85 $\pm$ 0.01	11.48 $\pm$ 0.01(24.9)
Arp 82B	B	21.9 $\pm$ 1.2	15.15 $\pm$ 0.02	10.5 $\pm$ 0.3	22.82 $\pm$ 0.01	14.84 $\pm$ 0.01(26.9)	-18.90
	V	29.1 $\pm$ 0.9	14.35 $\pm$ 0.01	10.5 $\pm$ 0.3	22.17 $\pm$ 0.01	14.14 $\pm$ 0.01(26.4)
	R	33.6 $\pm$ 0.9	13.86 $\pm$ 0.01	10.0 $\pm$ 0.3	21.65 $\pm$ 0.01	13.72 $\pm$ 0.01(26.4)
	I	48.9 $\pm$ 2.1	13.08 $\pm$ 0.01	10.5 $\pm$ 0.3	20.99 $\pm$ 0.00	13.01 $\pm$ 0.01(25.1)
Kar 168A	B	83.0 $\pm$ 4.5	12.20 $\pm$ 0.04	24.6 $\pm$ 0.3	22.24 $\pm$ 0.02	12.04 $\pm$ 0.07	-20.10
	V	88.0 $\pm$ 4.8	11.65 $\pm$ 0.04	20.8 $\pm$ 0.3	21.29 $\pm$ 0.01	11.57 $\pm$ 0.04
	R	102.1 $\pm$ 2.9	11.08 $\pm$ 0.03	20.8 $\pm$ 0.3	20.75 $\pm$ 0.00	11.01 $\pm$ 0.03
	I	113.0 $\pm$ 6.7	10.80 $\pm$ 0.02	21.4 $\pm$ 0.3	20.60 $\pm$ 0.01	10.75 $\pm$ 0.04
Kar 168B	B	27.9 $\pm$ 2.4	14.77 $\pm$ 0.04	15.2 $\pm$ 0.6	23.14 $\pm$ 0.05	14.43 $\pm$ 0.07	-17.90
	V	32.7 $\pm$ 2.0	14.47 $\pm$ 0.05	15.0 $\pm$ 0.3	22.94 $\pm$ 0.03	14.31 $\pm$ 0.07
	R	45.4 $\pm$ 2.5	13.80 $\pm$ 0.03	15.4 $\pm$ 0.3	22.59 $\pm$ 0.02	13.71 $\pm$ 0.04
	I	50.0 $\pm$ 3.2	13.63 $\pm$ 0.04	15.7 $\pm$ 0.3	22.52 $\pm$ 0.02	13.64 $\pm$ 0.04
Kar 179A	R	45.5 $\pm$ 1.4	13.31 $\pm$ 0.09	11.9 $\pm$ 0.2	21.85 $\pm$ 0.01	13.24 $\pm$ 0.11
Kar 179B	B	31.6 $\pm$ 0.4	14.66 $\pm$ 0.16	16.5 $\pm$ 0.4	23.40 $\pm$ 0.03	14.37 $\pm$ 0.11	-19.17
	V	43.0 $\pm$ 0.5	13.30 $\pm$ 0.12	14.6 $\pm$ 0.2	21.98 $\pm$ 0.00	13.18 $\pm$ 0.13
	R	48.5 $\pm$ 1.5	12.75 $\pm$ 0.08	14.3 $\pm$ 0.2	21.43 $\pm$ 0.01	12.67 $\pm$ 0.10

 

Table 2: continued

Galaxy	Filt	R25	m25	$r_{\rm e}$	$\mu_{\rm e}$	m	MB(corr)
Kar 203A	B	26.0 $\pm$ 4.6	13.88 $\pm$ 0.16	9.8 $\pm$ 1.0	21.20 $\pm$ 0.06	13.83 $\pm$ 0.16	-19.66
	V	24.0 $\pm$ 1.2	13.83 $\pm$ 0.08	9.5 $\pm$ 0.5	21.16 $\pm$ 0.01	13.81 $\pm$ 0.13
	R	25.7 $\pm$ 0.8	13.28 $\pm$ 0.06	9.5 $\pm$ 0.4	20.49 $\pm$ 0.00	13.26 $\pm$ 0.15
	I	31.0 $\pm$ 2.4	12.93 $\pm$ 0.14	10.2 $\pm$ 0.6	20.30 $\pm$ 0.02	12.91 $\pm$ 0.12
Kar 203B	V	37.0 $\pm$ 1.0	14.38 $\pm$ 0.04	19.2 $\pm$ 0.4	23.14 $\pm$ 0.04	14.20 $\pm$ 0.04
Kar 296B	B	31.8 $\pm$ 0.6	13.55 $\pm$ 0.04	13.5 $\pm$ 0.3	21.69 $\pm$ 0.01	13.49 $\pm$ 0.15	-19.75
	V	36.3 $\pm$ 1.5	12.74 $\pm$ 0.04	12.3 $\pm$ 0.6	20.84 $\pm$ 0.01	12.71 $\pm$ 0.09
	R	38.7 $\pm$ 1.2*	12.25 $\pm$ 0.08*	12.4 $\pm$ 0.3	20.32 $\pm$ 0.01	12.21 $\pm$ 0.08
	I	42.8 $\pm$ 1.0*	11.53 $\pm$ 0.05*	12.6 $\pm$ 0.6	19.66 $\pm$ 0.01	11.50 $\pm$ 0.09
Kar 296A	B	17.6 $\pm$ 1.2	14.63 $\pm$ 0.11	4.6 $\pm$ 0.3	20.59 $\pm$ 0.01	14.58 $\pm$ 0.15	-18.67
	V	19.4 $\pm$ 0.6*	13.94 $\pm$ 0.02*	4.3 $\pm$ 0.3	19.73 $\pm$ 0.00	13.90 $\pm$ 0.10
	R	20.6 $\pm$ 1.0*	13.55 $\pm$ 0.06*	4.6 $\pm$ 0.3	19.50 $\pm$ 0.01	13.52 $\pm$ 0.10
	I	24.0 $\pm$ 1.2*	12.75 $\pm$ 0.06*	4.5 $\pm$ 0.3	18.63 $\pm$ 0.00	12.72 $\pm$ 0.12
Arp 87A	B	36.0 $\pm$ 3.2	13.74 $\pm$ 0.07	14.7 $\pm$ 0.3	22.18 $\pm$ 0.02	13.52 $\pm$ 0.12(26.4)	-21.37
	V	38.2 $\pm$ 1.3	13.39 $\pm$ 0.06	14.1 $\pm$ 0.3	21.80 $\pm$ 0.01	13.21 $\pm$ 0.11(26.4)
	R	42.5 $\pm$ 0.6	12.70 $\pm$ 0.06	12.9 $\pm$ 0.7	21.02 $\pm$ 0.00	12.62 $\pm$ 0.21(27.2)
	I	43.5 $\pm$3.5	12.48 $\pm$ 0.30	12.1 $\pm$ 0.7	20.85 $\pm$ 0.01	12.46 $\pm$ 0.21(26.1)
Arp 87B	B	23.0 $\pm$ 0.9	14.60 $\pm$ 0.08	6.1 $\pm$ 0.3	21.52 $\pm$ 0.01	14.48 $\pm$ 0.33	-20.45
	V	25.3 $\pm$ 1.0	14.20 $\pm$ 0.07	6.4 $\pm$ 0.3	21.25 $\pm$ 0.01	14.09 $\pm$ 0.20
	R	34.2 $\pm$ 1.5	13.36 $\pm$ 0.06	6.5 $\pm$ 0.3	20.54 $\pm$ 0.00	13.27 $\pm$ 0.14
	I	35.8 $\pm$ 2.6	13.12 $\pm$ 0.16	5.9 $\pm$ 0.3	20.00 $\pm$ 0.00	13.07 $\pm$ 0.20
Kar 302A	R	137.5 $\pm$ 2.3*	9.93 $\pm$ 0.03*	37.1 $\pm$ 1.9	20.71 $\pm$ 0.07	9.91 $\pm$ 0.22
	I	141.5 $\pm$ 2.9*	9.57 $\pm$ 0.04*	35.0 $\pm$ 1.7	20.35 $\pm$ 0.13	9.56 $\pm$ 0.12
Kar 302B	B	51.8 $\pm$ 3.2	13.27 $\pm$ 0.06	18.9 $\pm$ 0.4	22.64 $\pm$ 0.06	13.13 $\pm$ 0.15	-17.22
	V	63.0 $\pm$ 2.2	12.36 $\pm$ 0.10	21.8 $\pm$ 1.3	22.01 $\pm$ 0.10	12.28 $\pm$ 0.14
	R	60.2 $\pm$ 0.9	12.85 $\pm$ 0.04	22.1 $\pm$ 0.4	22.51 $\pm$ 0.03	12.72 $\pm$ 0.04
	I	64.0 $\pm$ 2.9	12.78 $\pm$0.11	24.6 $\pm$ 0.2	22.63 $\pm$ 0.09	12.66 $\pm$ 0.04
Kar 331A	B	34.0 $\pm$ 1.2*	13.68 $\pm$ 0.17*	6.6 $\pm$ 0.2	20.87 $\pm$ 0.04	13.60 $\pm$ 0.03	-20.18
Kar 331B	B	19.6 $\pm$ 1.8	15.47 $\pm$ 0.18	7.0 $\pm$ 0.2	22.68 $\pm$ 0.05	15.29 $\pm$ 0.43	-18.40
	V	23.8 $\pm$ 1.0	14.55 $\pm$ 0.12	6.6 $\pm$ 0.4	21.70 $\pm$ 0.02	14.46 $\pm$ 0.23
	R	25.6 $\pm$ 2.8	14.06 $\pm$ 0.12	6.0 $\pm$ 0.2	21.09 $\pm$ 0.02	14.01 $\pm$ 0.05
Arp 183	B	25.8 $\pm$ 0.1	15.24 $\pm$ 0.07	13.2 $\pm$ 0.2	23.52 $\pm$ 0.02	15.03 $\pm$ 0.12	-19.09
	V	33.4 $\pm$ 2.0	14.45 $\pm$ 0.07	14.3 $\pm$ 1.1	22.86 $\pm$ 0.04	14.34 $\pm$ 0.15
	R	35.4 $\pm$ 2.2	13.95 $\pm$ 0.06	14.2 $\pm$ 1.0	22.41 $\pm$ 0.04	13.88 $\pm$ 0.07
	I	37.6 $\pm$ 1.5*	13.61 $\pm$ 0.12*	14.0 $\pm$ 0.6	22.15 $\pm$0.08	13.55 $\pm$ 0.13
Arp 36	B	26.2 $\pm$ 1.8	15.96 $\pm$ 0.05	20.0 $\pm$ 1.2	24.86 $\pm$ 0.21	15.51 $\pm$ 0.33	-18.64
	V	31.2 $\pm$ 0.2	15.27 $\pm$ 0.03	20.2 $\pm$ 0.2	24.36 $\pm$ 0.03	15.00 $\pm$ 0.09
	R	34.2 $\pm$ 2.8	14.78 $\pm$ 0.05	19.2 $\pm$ 0.6	23.74 $\pm$ 0.03	14.62 $\pm$ 0.11
	I	43.2 $\pm$ 4.4	14.16 $\pm$ 0.10	23.4 $\pm$ 4.8	23.37 $\pm$ 0.30	13.95 $\pm$ 0.11
Kar 404A	B	37.8 $\pm$ 1.0	13.38 $\pm$ 0.06	13.6 $\pm$ 0.3	21.77 $\pm$ 0.01	13.08 $\pm$ 0.06(26.6)	-20.20
	V	51.2 $\pm$ 5.8	12.90 $\pm$ 0.04	14.5 $\pm$ 0.3	21.66 $\pm$ 0.02	12.63 $\pm$ 0.04(26.0)
	R	81.3 $\pm$ 20.0	12.06 $\pm$ 0.08	12.9 $\pm$ 1.1	20.56 $\pm$ 0.01	11.95 $\pm$ 0.08(25.5)
	I	109.8 $\pm$ 50.0	11.47 $\pm$ 0.18	11.3 $\pm$ 0.3	19.88 $\pm$ 0.02	11.45 $\pm$ 0.18(25.0)
Kar 404B	B	81.0 $\pm$ 1.6	11.93 $\pm$ 0.05	38.1 $\pm$ 0.3	22.52 $\pm$ 0.02	11.88 $\pm$ 0.27	-21.49
	V	87.4 $\pm$ 4.5	11.42 $\pm$ 0.03	38.7 $\pm$ 0.6	22.06 $\pm$ 0.04	11.35 $\pm$ 0.09
	R	104.0 $\pm$ 7.1	10.67 $\pm$ 0.06	38.1 $\pm$1.0	21.29 $\pm$ 0.02	10.61 $\pm$ 0.08
	I	108.0 $\pm$ 10.0	10.07 $\pm$ 0.19	36.5 $\pm$ 1.3	20.63 $\pm$ 0.04	10.05 $\pm$ 0.21

 

Table 2: continued

Galaxy	Filt	R25	m25	$r_{\rm e}$	$\mu_{\rm e}$	m	MB(corr)
NGC 5905	B	89.0 $\pm$ 0.7	12.86 $\pm$ 0.15	65.9 $\pm$ 15.0	24.41 $\pm$ 0.43	12.36 $\pm$ 0.07	-20.94
	V	96.5 $\pm$ 4.8	12.12 $\pm$ 0.05	41.0 $\pm$ 1.0	23.06 $\pm$ 0.04	11.96 $\pm$ 0.08
	R	100.8 $\pm$ 1.0	11.73 $\pm$ 0.06	35.8 $\pm$ 0.6	22.35 $\pm$ 0.01	11.62 $\pm$ 0.06
	I	128.0 $\pm$ 1.6*	10.94 $\pm$ 0.04*	36.7 $\pm$ 0.3	21.69 $\pm$ 0.01	10.87 $\pm$ 0.03
NGC 5908	B	69.4 $\pm$ 0.6	13.29 $\pm$ 0.08	42.6 $\pm$ 0.3	23.94 $\pm$ 0.02	12.97 $\pm$ 0.15	-20.28
	V	85.0 $\pm$ 4.5	12.21 $\pm$ 0.03	36.5 $\pm$ 2.6	22.76 $\pm$ 0.07	12.07 $\pm$ 0.07
	R	100.0 $\pm$ 1.0	11.45 $\pm$ 0.02	36.8 $\pm$ 0.3	22.07 $\pm$ 0.01	11.31 $\pm$ 0.04
	I	118.4 $\pm$ 15.0	10.63 $\pm$ 0.01	32.6 $\pm$ 0.9	21.11 $\pm$ 0.02	10.58 $\pm$ 0.02
Kar 471A	B	24.6 $\pm$ 2.6	14.60 $\pm$ 0.11	7.3 $\pm$ 0.2	21.80 $\pm$ 0.04	14.52 $\pm$ 0.27	-21.01
	V	29.6 $\pm$ 2.8	13.86 $\pm$ 0.09	7.8 $\pm$ 0.2	21.39 $\pm$ 0.02	13.80 $\pm$ 0.11
	R	37.0 $\pm$ 2.0	13.27 $\pm$ 0.11	8.6 $\pm$ 0.2	21.01 $\pm$ 0.01	13.21 $\pm$ 0.11
	I	37.4 $\pm$ 2.0	12.92 $\pm$ 0.16	9.0 $\pm$ 0.2	20.76 $\pm$ 0.02	12.86 $\pm$ 0.11
Kar 471B	B	33.6 $\pm$ 0.8	13.96 $\pm$ 0.08	12.0 $\pm$ 0.2	21.90 $\pm$ 0.02	13.89 $\pm$ 0.25	-21.66
	V	39.2 $\pm$ 2.4	13.29 $\pm$ 0.08	12.2 $\pm$ 0.2	21.38 $\pm$ 0.02	13.25 $\pm$ 0.13
	R	46.0 $\pm$ 4.4	12.87 $\pm$ 0.09	12.8 $\pm$ 0.2	21.21 $\pm$ 0.02	12.82 $\pm$ 0.10
	I	45.0 $\pm$ 2.8	12.47 $\pm$ 0.20	10.7 $\pm$ 0.2	20.29 $\pm$ 0.01	12.45 $\pm$ 0.25
Arp 218A	B	18.4 $\pm$ 0.2	16.27 $\pm$ 0.07	11.6 $\pm$ 0.4	23.92 $\pm$ 0.04	15.89 $\pm$ 0.34	-20.66
	V	26.4 $\pm$ 1.4	15.39 $\pm$ 0.04	12.4 $\pm$ 0.4	23.45 $\pm$ 0.06	15.21 $\pm$ 0.18
	R	27.4 $\pm$ 0.2	14.78 $\pm$ 0.05	11.5 $\pm$ 0.2	22.66 $\pm$ 0.04	14.66 $\pm$ 0.13
	I	27.2 $\pm$ 1.6	14.37 $\pm$ 0.12	9.8 $\pm$ 0.4	21.88 $\pm$ 0.02	14.30 $\pm$ 0.47
Arp 218B	B	7.8 $\pm$ 0.6	17.95 $\pm$ 0.10	4.2 $\pm$ 0.2	23.78 $\pm$ 0.04	17.72 $\pm$ 0.33	-18.83
	V	10.4 $\pm$ 1.0	16.93 $\pm$ 0.08	3.8 $\pm$ 0.2	22.81 $\pm$ 0.04	16.77 $\pm$ 0.45
	R	12.6 $\pm$ 1.4	16.18 $\pm$ 0.06	4.2 $\pm$ 0.2	22.11 $\pm$ 0.02	16.09 $\pm$ 0.12
	I	13.2 $\pm$ 1.2	15.53 $\pm$ 0.17	4.0 $\pm$ 0.2	21.32 $\pm$ 0.02	15.49 $\pm$ 0.30
Kar 523A	B	18.8 $\pm$ 1.4	15.43 $\pm$ 0.18	6.6 $\pm$ 0.4	22.65 $\pm$ 0.05	15.25 $\pm$ 0.33	-19.54
	V	22.2 $\pm$ 1.6	14.67 $\pm$ 0.08	5.7 $\pm$ 0.2	21.64 $\pm$ 0.02	14.68 $\pm$ 0.14
	R	25.8 $\pm$ 1.2	13.86 $\pm$ 0.10	5.8 $\pm$ 0.2	20.93 $\pm$ 0.01	13.81 $\pm$ 0.14
	I	32.3 $\pm$ 1.0*	13.14 $\pm$ 0.08*	5.8 $\pm$ 0.4	20.26 $\pm$ 0.03	13.13 $\pm$ 0.12
Kar 523B	B	30.6 $\pm$ 2.2	14.37 $\pm$ 0.16	10.4 $\pm$ 0.2	21.95 $\pm$ 0.03	14.26 $\pm$ 0.45	-20.64
	V	41.5 $\pm$ 4.8	13.43 $\pm$ 0.10	12.0 $\pm$ 0.4	21.75 $\pm$ 0.03	13.34 $\pm$ 0.12
	R	40.6 $\pm$ 3.6	12.94 $\pm$ 0.10	10.4 $\pm$ 0.2	20.69 $\pm$ 0.02	12.90 $\pm$ 0.15
	I	46.0 $\pm$ 8.8*	12.30 $\pm$ 0.22*	10.5 $\pm$ 0.2	20.14 $\pm$ 0.04	12.28 $\pm$ 0.22
Kar 538A	B	28.3 $\pm$ 3.8	14.13 $\pm$ 0.14	9.2 $\pm$ 1.4	21.72 $\pm$ 0.03	14.02 $\pm$ 0.45	-21.01
	I	57.8 $\pm$ 11.0*	12.314 $\pm$ 0.15*	11.4 $\pm$ 0.4	20.40 $\pm$ 0.04	12.18 $\pm$ 0.08
Kar 538B	B	19.1 $\pm$ 3.0	15.44 $\pm$ 0.35	7.2 $\pm$ 0.4	22.55 $\pm$ 0.12	15.29 $\pm$ 0.79	-19.75
	I	31.2 $\pm$ 12.0	12.80 $\pm$ 0.21	6.8 $\pm$ 0.2	19.86 $\pm$ 0.01	12.78 $\pm$ 0.22
Arp 298A	B	47.4 $\pm$ 0.4	13.03 $\pm$ 0.09	3.8 $\pm$ 0.3	19.95 $\pm$ 0.00	12.98 $\pm$ 0.34	-21.09
	V	58.0 $\pm$ 3.2	12.35 $\pm$ 0.04	15.0 $\pm$ 0.3	21.53 $\pm$ 0.00	12.30 $\pm$ 0.11
	R	61.5 $\pm$ 4.5	11.84 $\pm$ 0.06	9.9 $\pm$ 0.3	20.21 $\pm$ 0.01	11.81 $\pm$ 0.18
Arp 298B	B	25.0 $\pm$ 0.6	15.09 $\pm$ 0.09	14.1 $\pm$ 0.3	23.09 $\pm$ 0.01	14.78 $\pm$ 0.37	-19.32
	V	32.6 $\pm$ 2.5	13.90 $\pm$ 0.04	12.8 $\pm$ 0.3	21.88 $\pm$ 0.03	13.75 $\pm$ 0.30
	R	39.0 $\pm$ 3.8	13.45 $\pm$ 0.07	13.4 $\pm$ 0.3	21.59 $\pm$ 0.02	13.30 $\pm$ 0.12

* Extrapolated value.

Total magnitudes and effective surface brightnesses were generally determined by extrapolation to infinity. However, for peculiarly flat intensity profiles no extrapolation was made and in these cases the surface brightnesses used are shown in parenthesis. When the measurements were not deep enough to determine well the total magnitudes, the effective values are omitted. The absolute magnitudes are corrected for Galactic extinction and redshift, whereas for the apparent magnitudes no corrections were applied.

 

Table 3: Bulge-disk decomposition by model 1

Galaxy	f	$\sigma$	$\bigtriangleup$	$\mu_0$	h	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	B/D
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
Arp 70A	B	0.65	0.11	21.88	6.9	22.24	23.69	11.55	22.03	24.06	9.59	0.84*
	V	0.55	0.11	20.90	6.1	21.26	22.71	10.15	20.54	22.59	8.05	1.24*
	R	0.71	0.10	20.13	5.8	20.50	21.95	9.73	19.57	21.64	6.79	1.16*
	I	0.71	0.09	19.61	5.2	19.99	21.44	8.75	19.24	21.30	7.91	1.64*
Arp 70B	B	0.65	0.04	21.31	2.3	21.68	23.10	3.85	21.48	23.52	5.39	2.31*
	V	0.55	0.06	20.26	2.4	20.62	22.05	3.99	20.08	22.14	4.27	1.72*
	R	0.71	0.05	19.58	2.6	19.95	21.38	4.27	19.31	21.35	3.71	1.34*
	I	0.71	0.05	18.95	2.5	19.36	20.80	4.27	19.39	21.42	4.83	1.27*
Arp 74B	B	1.15	0.09	22.24	2.9	22.68	24.09	4.97	23.58	25.21	10.85	2.11
	V	1.15	0.04	20.99	3.3	21.41	22.83	5.67	23.19	24.77	11.55	0.81
	R	0.98	0.07	20.96	3.7	21.35	22.79	6.23	21.63	23.47	7.91	1.26
	I	0.68	0.06	20.42	3.2	20.80	22.24	5.39	21.17	22.92	9.45	2.19
Kar 64A	V	0.85	0.22	21.48	20.5	21.18	22.88	32.16	19.41	21.48	4.32	0.12
	R	0.64	0.25	20.88	20.0	21.18	22.59	31.52	19.90	22.00	7.84	0.20
	I	0.64	0.20	20.46	18.7	20.78	22.20	29.92	18.61	20.72	4.96	0.20
Kar 64B	V	0.85	0.10	20.93	9.8	21.29	22.75	16.48	19.74	21.08	1.12	0.02*
	R	0.64	0.09	20.60	9.8	20.96	22.42	16.48	22.38	24.48	9.76	0.10*
	I	0.64	0.09	20.45	10.5	20.80	22.25	17.44	19.76	21.84	4.00	0.14*
Kar 125A1	B	0.72	0.11	20.36	5.9	20.71	22.15	9.70	20.48	22.42	9.70	1.41
	V	0.72	0.06	19.88	5.4	20.23	21.68	8.90	19.56	21.46	10.30	2.93
	R	0.72	0.06	18.95	5.0	19.31	20.75	8.30	19.07	20.99	9.90	2.03
	I	0.55	0.07	18.99	5.5	19.34	20.78	9.00	18.16	20.11	9.30	3.46
Arp 82A	B	0.93	0.15	21.83	19.2	22.18	23.61	31.65	19.84	21.29	1.65	0.03*
	V	0.85	0.14	21.06	18.0	21.41	22.86	29.85	19.21	21.02	2.25	0.04*
	R	0.85	0.12	20.63	18.2	20.99	22.43	30.15	18.84	20.80	2.85	0.06*
	I	0.93	0.15	20.00	19.2	20.35	21.79	31.65	18.02	19.47	1.65	0.02*
Kar 179A	R	0.38	0.18	21.64	12.6	21.98	23.41	20.51	19.53	21.63	7.77	1.38
Kar 179B	B	0.42	0.10	22.20	10.1	22.56	24.00	16.73	21.98	23.99	12.81	1.00
	V	0.42	0.11	20.67	9.3	21.02	22.47	15.47	20.49	22.54	10.43	0.78
	R	0.49	0.10	20.07	9.1	20.44	21.89	15.19	19.97	22.03	10.29	0.74
Kar 203B	V	0.58	-	21.61	12.2	21.79	23.11	16.90	20.78	22.56	1.50	0.02
Kar 296B	B	0.38	0.06	19.98	6.6	20.32	21.77	10.95	23.60	25.34	16.05	0.15
	V	0.38	0.08	18.94	6.5	19.27	20.72	10.65	26.88	27.90	28.95	0.06
Kar 296A	B	0.38	0.09	19.65	3.2	19.96	21.42	5.25	21.33	23.34	5.85	0.38
	V	0.38	0.09	18.96	3.1	19.26	20.71	4.95	19.96	22.01	4.95	0.54
	R	0.38	0.09	18.47	2.9	18.82	20.29	4.95	19.71	21.72	5.55	0.62
	I	0.38	0.08	17.94	3.1	18.24	19.68	4.95	18.51	20.54	4.95	0.82
Arp 87A	B	0.65	0.08	20.20	8.0	20.55	21.99	13.28	20.83	22.31	1.12	0.01*
	V	0.65	0.09	19.88	7.9	20.24	21.69	13.28	20.27	22.29	2.32	0.04*
	R	0.84	0.10	19.20	7.8	19.55	20.99	12.96	19.29	21.25	3.04	0.07*
	I	0.89	0.11	19.00	7.7	19.36	20.82	12.96	18.84	20.86	3.36	0.11*
Arp 87B	B	0.65	0.30	21.09	4.9	21.43	22.88	8.16	20.26	22.39	6.56	1.89
	V	0.65	0.19	20.65	4.7	20.99	22.45	7.84	19.84	21.96	6.56	2.05
	R	0.84	0.16	-	-		-	-	18.58	20.68	6.56	-
	I	0.89	0.11	19.21	3.4	19.57	21.01	5.6	18.78	20.88	6.88	3.16
Kar 302A	R	0.73	0.11	19.00	24.0	19.32	20.74	38.6	19.25	21.32	16.48	0.20
	I	0.68	0.10	18.60	23.4	18.93	20.35	37.6	18.64	20.72	15.52	0.22
Kar 302B	B	0.73	0.16	21.48	13.0	21.84	23.29	21.6	21.32	23.35	17.44	1.12
	V	0.64	0.15	20.48	13.8	20.84	22.29	22.9	21.16	23.15	20.96	0.68
	R	0.64	0.14	21.14	14.8	21.49	22.94	24.5	21.41	23.42	19.36	0.73
	I	0.51	0.17	21.21	15.8	21.56	23.00	26.1	21.61	23.59	21.92	0.74
Kar 331A2	B	1.02	0.06	19.38	3.1	19.79	21.22	5.3	19.88	21.83	8.30	2.57
Kar 331B	B	0.85	0.14	21.73	4.3	22.10	23.55	7.3	21.39	23.38	7.70	2.37
	V	0.85	0.15	21.03	5.5	21.39	22.84	9.1	20.09	22.11	5.50	1.28
	R	0.85	0.16	20.37	5.5	20.73	22.17	9.1	18.85	20.85	3.50	0.84
Arp 183	B	0.72	0.12	21.87	6.4	22.21	23.65	10.50	23.10	24.71	15.90	1.68
	V	0.72	0.08	21.70	8.2	22.00	23.40	12.90	22.19	23.86	14.70	1.61
	R	0.37	0.09	21.18	9.2	21.45	22.84	14.10	21.70	23.48	12.50	0.79
	I	0.37	0.08	21.03	9.4	21.30	22.68	14.30	21.15	22.94	12.50	1.10

 

Table 3: continued

Galaxy	f	$\sigma$	$\bigtriangleup$	$\mu_0$	h	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	B/D
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
Arp 36	B	0.34	0.15	23.14	11.6	23.43	24.83	18.10	24.40	26.26	14.30	0.30
	R	0.29	0.14	22.00	11.1	22.31	23.72	17.50	23.74	25.70	11.30	0.12
	I	0.29	0.11	22.07	15.1	22.29	23.63	21.70	23.12	24.86	18.10	0.41
Kar 404A	B	0.62	0.09	21.18	10.8	21.54	22.99	18.08	18.53	20.63	3.68	0.66*
	V	0.54	0.10	21.39	12.9	21.75	23.21	21.60	18.56	20.70	5.28	1.12*
	R	0.64	0.08	21.78	16.4	22.14	23.60	27.36	18.10	20.23	7.20	2.86*
	I	0.55	0.09	21.47	15.2	21.82	23.27	25.12	17.28	19.41	6.56	4.42*
NGC 5905*	B	0.81	0.06	23.05	51.1	23.17	24.44	65.44	20.80	22.92	10.72	0.20
	V	0.55	0.08	21.73	31.5	22.03	23.43	49.12	19.40	21.52	7.84	0.28
	R	0.70	0.06	21.34	29.4	21.64	23.05	46.24	19.02	21.15	8.80	0.39
	I	0.70	0.06	21.01	33.5	21.28	22.66	51.04	18.67	20.78	12.00	0.59
Kar 471A	B	0.55	0.17	20.91	6.1	21.25	22.69	10.10	19.42	21.48	3.10	0.52
	V	0.55	0.14	20.35	6.6	20.69	22.13	10.90	18.84	20.91	3.30	0.51
	R	0.55	0.09	20.76	6.4	21.09	22.53	10.50	19.25	21.25	7.70	3.18
	I	0.55	0.08	20.64	7.8	20.96	22.38	12.50	18.79	20.80	7.10	2.51
Arp 218B	B	0.42	0.15	22.18	2.8	22.49	23.93	4.50	22.30	24.37	2.10	0.25
	V	0.42	0.14	21.58	3.1	21.92	23.37	5.10	21.48	23.56	2.70	0.42
	R	0.42	0.08	20.54	2.4	20.85	22.29	3.90	22.11	24.07	5.90	0.80
	I	0.32	0.11	19.63	2.4	19.99	21.46	4.10	21.19	23.25	3.30	0.23
Kar 523A	B	0.30	0.20	22.07	6.4	22.40	23.85	10.50	19.92	22.03	3.50	1.11
	V	0.50	0.08	21.46	6.0	21.80	23.24	9.90	18.99	21.07	3.30	1.49
	R	0.36	0.12	20.26	5.7	20.61	22.06	9.50	17.73	19.81	2.30	0.86
	I	0.45	0.07	20.30	6.2	20.65	22.10	10.30	17.77	19.85	3.90	2.11
Kar 523B	B	0.35	0.23	21.49	8.0	21.83	23.27	13.10	21.10	23.12	8.10	0.80
	V	0.37	0.11	21.58	8.5	21.91	23.34	13.70	20.48	22.39	12.10	3.35
	R	0.35	0.16	20.25	8.5	20.57	21.99	13.70	19.48	21.53	7.30	0.80
	I	0.30	0.16	19.90	8.9	20.23	21.65	14.30	18.92	20.95	8.30	1.18
Kar 538A	B	0.35	0.20	20.59	4.2	20.93	22.37	6.90	20.51	22.52	8.70	2.50
Kar 538B	B	0.28	0.18	21.33	4.5	21.68	23.13	7.5	21.90	23.92	8.7	1.19
	I	0.30	0.18	19.06	4.7	19.41	20.87	7.9	18.66	20.73	6.5	1.42
Arp 298A3	B	0.66	0.26	17.68	7.4	24.49	24.76	40.80	16.54	18.70	3.04	8.50
	V	0.66	0.18	15.00	6.5	23.71	23.83	43.68	16.50	18.63	4.32	7.70
	R	0.72	0.14	14.80	6.5	23.23	23.36	42.40	16.53	18.67	4.96	6.63
Arp 298B	B	0.66	0.13	21.81	7.8	22.17	23.62	12.96	25.12	26.71	31.84	0.70
	V	0.66	0.13	20.70	7.0	21.06	22.51	11.68	22.70	24.58	20.32	0.81
	R	0.72	0.06	20.22	6.9	20.55	22.00	11.36	22.71	24.49	24.48	0.83

(1) Galaxy. When marked by an asterisk, model 1 gives a better fit than model 2.

(2) Filter.

(3) Dispersion $\sigma$ of the Gaussian point spread function, measured from the foreground stars in the images [arcsec].

(4) The unweighted rms residual of the fit: $\bigtriangleup^2=\sum(\mu_i - \mu_{\rm fit})^2/N$

(5) The central surface brightness [mag arcsec^-2].

(6) The disk scalelength [arcsec].

(7) The mean effective surface brightness of the disk [mag arcsec^-2].

(8) The effective surface brightness of the disk [mag arcsec^-2].

(9) The effective radius of the disk [arcsec].

(10) The mean effective surface brightness of the bulge [mag arcsec^-2].

(11) The effective surface brightness of the bulge [mag arcsec^-2].

(12) The effective radius of the bulge [arcsec].

(13) The bulge/disk ratio. Generally the value is obtained by extrapolating to infinity, but when marked by an asterisk no extrapolation was done.

¹ The image of Kar 125 B was not deep enough for bulge-to-disk decomposition.

² For Kar 331 A no reasonable fit was obtained in V, R and I-bands and the I-band for Kar 331 B is not of good enough quality for the bulge-to-disk decomposition.

³ Instead of model 1 model 3 was used.

 

Table 4: Bulge-disk decomposition by model 2

Galaxy	f	$\bigtriangleup$	$\mu_0$	h	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	B/D
Arp 70A	B	0.09	21.47	7.1	21.83	23.28	11.83	20.16	21.51	2.03	0.14*
	V	0.08	20.46	6.5	20.81	22.26	10.85	18.79	20.18	2.03	0.23*
	R	0.08	19.73	6.2	20.09	21.53	10.29	18.06	19.40	2.03	0.26*
	I	0.07	19.28	6.2	19.64	21.09	10.24	17.68	19.06	2.30	0.31*
Arp 70B	B	0.04	21.40	3.5	21.76	23.20	5.81	20.07	21.39	1.75	0.43*
	V	0.02	20.22	3.3	20.58	22.02	5.39	18.70	20.04	1.47	0.43*
	R	0.02	19.48	3.1	19.86	21.30	5.25	18.30	19.63	1.61	0.39*
	I	0.02	19.05	3.3	19.41	20.84	5.39	18.07	19.40	1.75	0.36*
Arp 74A*	B	0.09	22.57	16.0	22.79	24.13	23.03	20.86	22.12	2.17	0.05
	V	0.08	21.55	15.0	21.80	23.16	22.19	20.51	21.84	3.15	0.06
	R	0.07	20.81	13.2	21.10	22.48	20.37	19.33	20.62	2.03	0.05
	I	0.10	20.37	14.2	20.63	22.01	21.35	18.93	20.32	2.45	0.06
Arp 74B*	B	0.10	23.94	9.4	24.10	25.39	12.67	22.01	23.39	4.13	0.66
	V	0.04	23.47	10.3	23.60	24.86	13.23	21.11	22.52	5.11	1.24
	R	0.07	21.96	7.0	22.23	23.60	10.57	20.35	21.75	3.85	0.71
	I	0.06	21.63	8.5	21.83	23.16	11.97	19.71	21.15	3.71	0.61
Kar 64A	V	0.20	21.12	20.2	21.42	22.83	31.84	18.78	20.14	2.72	0.09
	R	0.21	20.77	19.7	21.08	22.49	31.20	18.72	20.18	3.68	0.12
	I	0.18	20.37	18.4	20.69	22.10	29.28	17.90	19.33	3.04	0.14
Kar 64B	B	0.06	22.35	12.1	22.64	24.03	18.69	23.11	24.29	1.47	0.01*
	V	0.08	20.93	9.9	21.29	22.74	16.48	19.79	21.05	1.12	0.02*
	R	0.06	20.54	9.8	20.91	22.36	16.48	20.29	21.66	2.08	0.03*
	I	0.08	20.23	9.8	20.58	22.03	16.16	18.42	19.80	1.44	0.06*
Kar 125A	B	0.07	20.70	8.5	21.00	22.41	13.50	19.00	20.45	4.30	0.61
	V	0.07	20.01	8.9	20.30	21.71	13.90	18.06	19.48	3.90	0.61
	R	0.07	19.68	9.2	19.97	21.37	14.30	17.52	18.94	4.30	0.85
	I	0.10	19.39	10.6	19.65	21.03	15.90	16.75	18.20	4.30	0.98
Arp 82A	B	0.14	21.83	19.2	22.18	23.61	31.65	19.87	21.16	1.65	0.02*
	V	0.13	21.04	17.9	21.39	22.84	29.55	19.02	20.41	1.95	0.04*
	R	0.11	20.60	18.0	20.95	22.39	29.85	18.34	19.68	1.95	0.05*
	I	0.14	20.00	19.2	20.35	21.79	31.65	18.05	19.33	1.65	0.02*
Arp 82B *	B	0.07	24.55	21.89	24.69	25.98	28.65	20.91	22.37	7.65	2.26*
	V	0.05	23.09	15.67	23.34	24.72	23.55	20.15	21.61	7.05	1.66*
	R	0.05	22.40	13.87	22.70	24.10	21.75	19.65	21.11	6.75	1.57*
	I	0.07	22.73	21.89	22.87	24.15	28.65	19.09	20.55	7.65	2.26*
Kar 168A*	B	0.13	21.91	29.2	22.24	23.66	46.88	18.99	20.43	8.80	0.69
	V	0.16	21.09	24.4	21.44	22.87	40.16	18.24	19.24	8.46	0.74
	R	0.16	20.68	25.8	21.02	22.45	42.08	17.77	19.19	8.16	0.78
	I	0.10	20.63	28.1	20.96	22.39	45.28	17.64	19.09	9.12	0.85
Kar 168B*	B	0.15	21.79	10.7	22.10	23.52	17.12	20.03	21.45	2.72	0.16
	V	0.15	21.49	10.1	21.82	23.26	16.48	20.14	21.55	3.04	0.16
	R	0.13	21.00	10.0	21.33	22.76	16.16	19.60	21.01	3.04	0.17
	I	0.12	20.31	10.6	20.64	22.07	17.20	19.08	20.54	4.00	0.23
Kar 179A	R	0.19	21.17	12.7	21.50	22.93	20.65	18.62	20.08	3.99	0.52
Kar 179B	B	0.04	21.78	10.6	22.13	23.57	17.57	20.12	21.56	3.01	0.19
	V	0.04	20.37	9.8	20.73	22.18	16.31	18.74	20.19	2.87	0.19
	R	0.04	19.82	9.6	20.18	21.63	16.03	18.24	19.67	2.87	0.19

 

Table 4: continued

Galaxy	f	$\bigtriangleup$	$\mu_0$	h	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	B/D
Kar 203A*1	B	0.18	18.37	4.0	21.09	21.87	11.90	19.56	21.01	4.70	0.64
	V	0.16	18.37	4.0	21.26	22.01	12.30	19.67	21.10	5.50	0.88
	R	0.18	17.89	4.0	20.78	21.53	12.30	19.06	20.51	5.50	0.98
	I	0.45	17.35	4.0	20.23	20.99	12.30	18.55	20.00	4.90	0.76
Kar 203B	V	0.10	21.61	12.2	21.79	23.11	16.90	20.41	21.68	1.10	0.01
Kar 296B*2	B	0.25	19.72	6.6	20.06	21.52	10.95	50.30	51.76	1.65	-
	V	0.08	19.00	6.6	19.35	20.81	10.95	50.25	51.79	1.65	-
	R	0.35	18.37	6.6	18.71	20.17	10.95	50.25	51.79	1.65	-
Kar 296A*	B	0.11	21.13	4.9	21.45	22.90	7.95	19.46	20.90	3.75	1.43
	V	0.11	20.12	4.6	20.43	21.87	7.35	18.48	19.92	3.15	1.12
	R	0.09	20.77	5.9	21.08	22.50	9.45	18.23	19.71	4.05	2.39
	I	0.09	20.06	6.2	20.36	21.78	9.75	17.47	18.94	4.05	2.34
Arp 87A	B	0.08	20.20	8.0	20.55	21.99	13.28	20.81	22.20	1.12	0.01*
	V	0.09	19.85	7.9	20.19	21.63	12.96	19.41	20.79	1.44	0.02*
	R	0.10	19.16	7.8	19.51	20.97	12.96	18.60	19.95	1.76	0.04*
	I	0.11	18.95	7.7	19.32	20.78	12.96	18.20	19.58	2.08	0.07*
Arp 87B *	B	0.27	21.85	8.2	22.21	23.66	13.60	19.27	20.70	3.68	1.12
	V	0.16	21.71	8.7	22.07	23.52	14.56	18.95	20.39	4.00	1.34
	R	0.13	21.51	11.0	21.87	23.32	18.40	18.22	19.66	4.32	1.58
	I	0.23	20.75	8.8	21.10	22.55	14.56	17.73	19.15	3.68	1.43
Kar 302A	R	0.11	18.89	24.1	19.22	20.65	38.88	17.65	19.09	5.28	0.08
	I	0.11	18.49	23.4	18.82	20.25	37.92	17.11	18.55	5.28	0.09
Kar 302B*	B	0.09	21.55	16.4	21.89	23.34	27.04	19.77	21.21	6.24	0.37
	V	0.07	20.45	15.8	20.81	22.25	26.08	19.36	20.81	5.92	0.20
	R	0.08	21.28	18.0	21.62	23.06	29.60	19.84	21.31	7.20	0.30
	I	0.10	21.14	18.1	21.48	22.92	29.60	19.84	21.28	6.24	0.20
Kar 331A*	B	0.09	21.22	9.2	21.50	22.89	14.10	18.57	19.99	4.10	1.16
	V	0.11	20.75	14.2	20.86	22.14	18.10	17.47	18.87	3.70	0.82
	R	0.12	20.13	13.4	20.27	21.56	17.70	16.84	18.25	3.50	0.81
	I	0.12	19.33	12.8	19.49	20.80	17.30	16.08	17.51	3.50	0.82
Kar 331B*	B	0.10	22.10	7.3	22.45	23.88	11.90	20.14	21.56	3.30	0.62
	V	0.08	20.97	6.5	21.31	22.75	10.70	19.19	20.59	2.90	0.50
	R	0.11	20.31	5.9	20.68	22.12	9.90	18.39	19.78	2.50	0.51
Arp 183	B	0.12	22.68	11.8	22.88	24.21	16.70	21.64	23.09	6.50	0.42
	V	0.11	21.23	9.4	21.50	22.88	14.30	20.70	22.11	2.50	0.06
	R	0.09	20.91	10.0	21.17	22.55	15.10	20.18	21.65	3.10	0.10
	I	0.07	20.67	10.4	20.92	22.29	15.50	19.63	21.07	3.10	0.12
Arp 36*	B	0.12	23.03	12.1	23.31	24.71	18.70	22.58	24.04	3.30	0.06
	V	0.09	22.52	12.3	22.80	24.19	18.90	22.15	23.62	3.30	0.05
	R	0.12	21.97	11.3	22.27	23.67	17.70	21.83	23.28	2.90	0.04
	I	0.08	21.88	15.6	22.09	23.42	22.10	21.44	22.91	3.90	0.05
Kar 404A	B	0.19	20.81	10.0	21.17	22.63	16.80	17.63	18.98	1.76	0.31*
	V	0.21	20.81	11.6	21.17	22.62	19.36	17.51	18.98	2.40	0.42*
	R	0.18	20.40	12.5	20.76	22.21	20.96	16.65	18.03	2.40	0.62*
	I	0.18	19.83	11.6	20.19	21.64	19.36	15.94	17.36	2.40	0.79*

 

Table 4: continued

Galaxy	f	$\bigtriangleup$	$\mu_0$	h	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	$m\mu_{\rm e}$	$\mu_{\rm e}$	$r_{\rm e}$	B/D
Kar 404B*	B	0.18	20.43	17.7	20.78	22.22	29.28	19.22	20.60	2.08	0.02
	V	0.12	20.15	20.6	20.50	21.95	34.08	18.60	20.04	3.04	0.05
	R	0.14	19.43	20.7	19.77	21.21	34.08	17.79	19.22	3.36	0.06
	I	0.13	18.67	18.8	19.03	20.48	31.20	16.94	18.37	3.04	0.07
NGC 5905	B	0.14	22.72	44.4	22.90	24.21	60.96	19.63	21.08	4.64	0.10
	V	0.14	21.46	29.3	21.76	23.17	46.24	18.38	19.81	3.68	0.14
	R	0.13	21.03	27.4	21.35	22.35	44.00	17.94	19.35	4.00	0.19
	I	0.15	20.58	30.5	20.88	22.28	47.84	17.45	18.88	4.96	0.25
Kar 471A	B	0.18	20.78	6.3	21.12	22.56	10.30	18.91	20.35	2.10	0.30
	V	0.15	20.21	6.7	20.54	21.98	10.90	18.26	19.66	2.10	0.30
	R	0.13	20.34	8.6	20.65	22.07	13.70	18.08	19.50	3.10	0.55
	I	0.13	19.94	8.6	20.25	21.66	13.70	17.67	19.11	2.90	0.47
Kar 471B*	B	0.20	20.34	7.6	20.68	22.12	12.50	19.68	21.08	0.70	0.01
	V	0.19	19.72	7.9	20.05	21.49	12.90	18.27	19.77	0.70	0.02
	R	0.20	19.56	8.5	19.90	21.34	13.90	18.19	19.71	1.10	0.03
	I	0.18	18.81	7.5	19.15	20.59	12.30	17.64	19.16	1.30	0.04
Arp 218A*1	B	0.11	22.22	7.4	23.17	24.35	14.30	22.85	24.32	6.7	0.28
	V	0.13	21.51	7.4	22.46	23.64	14.30	21.63	23.08	4.9	0.25
	R	0.11	20.99	7.4	21.95	23.13	14.30	20.87	22.33	4.9	0.31
	I	0.19	20.11	6.0	21.28	22.43	12.50	19.81	21.28	3.3	0.27
Arp 218B	B	0.14	22.08	2.8	22.43	23.89	4.70	21.20	22.56	0.90	0.11
	V	0.13	21.49	3.2	21.82	23.27	5.30	20.29	21.64	1.10	0.19
	R	0.08	21.63	3.9	21.98	23.43	6.70	20.25	21.68	2.50	0.74
	I	0.11	19.67	2.6	20.01	21.46	4.30	19.56	21.02	1.10	0.10
Kar 523A	B	0.18	21.54	6.1	21.88	23.33	10.10	18.78	20.22	1.50	0.39
	V	0.09	20.95	6.1	21.30	22.75	10.10	18.15	19.55	1.70	0.52
	R	0.08	19.98	5.7	20.31	21.75	9.30	17.21	18.64	1.50	0.45
	I	0.09	19.55	6.2	19.91	21.36	10.30	16.69	18.10	1.70	0.53
Kar 523B	B	0.19	21.56	9.5	21.90	23.28	15.10	19.80	21.24	3.30	0.32
	V	0.14	21.19	12.2	21.45	22.83	18.30	19.07	20.51	3.90	0.39
	R	0.16	20.18	9.4	20.49	21.91	15.10	18.33	19.80	3.30	0.34
	I	0.15	19.72	10.1	20.02	21.42	15.90	17.65	19.10	3.30	0.37
Kar 538A	B	0.17	22.02	10.4	22.31	23.70	16.10	19.04	20.49	3.70	1.03
	I	0.14	21.07	16.8	21.19	22.46	21.50	17.41	18.85	3.90	0.92
Kar 538B	B	0.19	21.21	5.5	21.55	22.99	9.10	18.49	19.90	0.70	0.10
	I	0.21	18.81	5.8	19.16	20.62	9.70	15.89	17.38	0.90	0.18
Arp 298B	B	0.10	25.39	28.1	25.51	26.78	36.00	22.00	23.46	12.32	2.49
	V	0.05	23.30	18.2	23.58	24.97	28.00	20.51	21.97	9.76	1.94
	R	0.08	23.77	29.1	23.87	25.13	36.64	20.18	21.63	10.72	2.15

The parameters are as in Table 3. Gaussian sigmas shown in Table 3 were used. Galaxies which had the best fit by model 2 are denoted by an asterisk.

¹ Instead of model 2, model 4 was used.

² The best fit was obtained by using a single exponential function.

Figure 2: The radial profiles of the position angle PA and the ellipticity $\epsilon$. The band used is denoted in parenthesis. The profiles were extracted from the original measurements with 1'' bins, by applying the isophotal fitting routine explained in the text (see Sect. 4.1). The errors were estimated using the Fourier-technique by Rauscher (1995) based on calculating the harmonic coefficients and the rms residual of the intensity. The values corresponding to the orientation estimated in Sect. 3 are denoted by vertical bars in the right-hand y-axis

Figure 2: continued

Figure 2: continued

Figure 2: continued

Figure 2: continued

Figure 3: Surface brightness profiles in the B, V, R and I-bands. The profiles were obtained by the elliptical averaging routine explained in the text (Sect. 4.2). In the figures the original profiles were rebinned by a factor 4. The error bar takes into account the background noise and global variations in the sky brightnesses. The global sky variation was taken to be $\pm$ 1/4 of the minimum - maximum sky brightnesses

Figure 3: continued

Figure 3: continued

Figure 3: continued

Figure 4: Bulge-disk decompositions of the surface brightness profiles presented in Fig. 3. The symbols indicate the measured profiles, the dash dotted line the fitted disk, and the dashed line the fitted bulge, whereas the dotted line shows the residuals between the observed data and the fitted profile. The zero-point of the residual is plotted at 28 mag arcsec-2. The bar below the image indicates the region used in the fit. The models take into account the observed seeing. We generally present the model where both the disk and the bulge are represented by an exponential (EE = model 2), but if the profile was better fitted by some other model the best fit is shown (S = single exponential; EEt = model 4; deVEt = model 3; deVE = model 1)

Figure 4: continued

Figure 4: continued

Figure 4: continued