Table 5: Results for the broad-band optical/ NIR photometry of our WR galaxies sample. E(B-V) was determined from the C(H$\beta $) calculated from our optical spectra. All magnitudes and colors have been corrected for extinction; optical colors have been also corrected for the emission of the ionized gas. Except for NGC 5253, absolute magnitudes were computed using the distances provided by our optical spectra. See figures for the identification of the different regions inside galaxies.

Object
E(B-V) mB MB U-B B-V V-R V-J J-H $H-K_{\rm s}$

HCG 31d
                 
ACc,d 0.06 $\pm$ 0.02 14.17 $\pm$ 0.05 -19.43 $\pm$ 0.05 -0.60 $\pm$ 0.06 0.03 $\pm$ 0.08 0.12 $\pm$ 0.08 0.20 $\pm$ 0.10 0.13 $\pm$ 0.10 0.15 $\pm$ 0.12
Bc 0.18 $\pm$ 0.04 14.89 $\pm$ 0.05 -18.71 $\pm$ 0.05 -0.38 $\pm$ 0.08 0.17 $\pm$ 0.06 0.06 $\pm$ 0.06 0.14 $\pm$ 0.10 0.13 $\pm$ 0.10 0.12 $\pm$ 0.10
Ec 0.06 $\pm$ 0.03 17.84 $\pm$ 0.06 -15.76 $\pm$ 0.06 -0.65 $\pm$ 0.10 -0.03 $\pm$ 0.10 0.20 $\pm$ 0.09 0.29 $\pm$ 0.12 0.05 $\pm$ 0.10 0.18 $\pm$ 0.12
F1c 0.20 $\pm$ 0.03 17.84 $\pm$ 0.06 -15.76 $\pm$ 0.06 -0.99 $\pm$ 0.12 -0.07 $\pm$ 0.12 -0.04 $\pm$ 0.10 -0.17 $\pm$ 0.14 0.04 $\pm$ 0.17 0.29 $\pm$ 0.30
F2c 0.09 $\pm$ 0.03 19.26 $\pm$ 0.06 -14.34 $\pm$ 0.06 -1.01 $\pm$ 0.12 -0.09 $\pm$ 0.12 -0.02 $\pm$ 0.10 0.01 $\pm$ 0.16 0.08 $\pm$ 0.30 0.20 $\pm$ 0.50
Gc 0.06 $\pm$ 0.03 14.72 $\pm$ 0.05 -18.88 $\pm$ 0.05 -0.43 $\pm$ 0.09 -0.01 $\pm$ 0.08 0.14 $\pm$ 0.08 0.45 $\pm$ 0.08 0.12 $\pm$ 0.10 0.13 $\pm$ 0.10
ACUC 0.06 $\pm$ 0.02 ... ... -0.38 $\pm$ 0.12 0.19 $\pm$ 0.10 0.29 $\pm$ 0.12 0.69 $\pm$ 0.14 0.53 $\pm$ 0.16 0.17 $\pm$ 0.16
BUC 0.18 $\pm$ 0.04 ... ... -0.27 $\pm$ 0.12 0.31 $\pm$ 0.08 0.23 $\pm$ 0.08 0.72 $\pm$ 0.10 0.61 $\pm$ 0.14 0.19 $\pm$ 0.16
GUC 0.06 $\pm$ 0.02 ... ... -0.33 $\pm$ 0.10 0.28 $\pm$ 0.08 0.30 $\pm$ 0.08 0.79 $\pm$ 0.10 0.52 $\pm$ 0.14 0.23 $\pm$ 0.16

Mkn 1087d
0.17a 13.08 $\pm$ 0.04 -22.15 $\pm$ 0.04 -0.41 $\pm$ 0.08 0.17 $\pm$ 0.08 0.20 $\pm$ 0.08 0.52 $\pm$ 0.06 0.20 $\pm$ 0.06 0.16 $\pm$ 0.06
Cc 0.14 $\pm$ 0.02 14.62 $\pm$ 0.03 -20.61 $\pm$ 0.03 -0.57 $\pm$ 0.06 -0.02 $\pm$ 0.06 0.11 $\pm$ 0.06 0.31 $\pm$ 0.10 0.15 $\pm$ 0.10 0.15 $\pm$ 0.10
N Compc 0.10 $\pm$ 0.02 17.17 $\pm$ 0.03 -18.06 $\pm$ 0.03 ... -0.05 $\pm$ 0.06 0.14 $\pm$ 0.10 0.21 $\pm$ 0.08 0.18 $\pm$ 0.08 0.13 $\pm$ 0.08
#1 0.07a 18.89 $\pm$ 0.05 -16.34 $\pm$ 0.05 -0.75 $\pm$ 0.15 -0.01 $\pm$ 0.10 0.10 $\pm$ 0.08 ... ... ...
#3 0.07a 18.03 $\pm$ 0.03 -17.20 $\pm$ 0.03 0.08 $\pm$ 0.30 0.11 $\pm$ 0.06 0.26 $\pm$ 0.06 0.64 $\pm$ 0.10 0.50 $\pm$ 0.20 ...
UC 0.17a ... ... ... 0.27 $\pm$ 0.08 0.29 $\pm$ 0.08 0.82 $\pm$ 0.10 0.59 $\pm$ 0.14 0.27 $\pm$ 0.16

Haro 15c
0.11a 13.82 $\pm$ 0.04 -20.87 $\pm$ 0.04 -0.52 $\pm$ 0.08 0.26 $\pm$ 0.08 0.32 $\pm$ 0.08 0.17 $\pm$ 0.08 0.58 $\pm$ 0.08 0.22 $\pm$ 0.08
Ac 0.23 $\pm$ 0.02 17.56 $\pm$ 0.04 -17.13 $\pm$ 0.04 -0.86 $\pm$ 0.10 -0.10 $\pm$ 0.08 0.13 $\pm$ 0.08 0.20 $\pm$ 0.08 0.24 $\pm$ 0.08 0.18 $\pm$ 0.10
B 0.04 $\pm$ 0.02 17.72 $\pm$ 0.04 -16.97 $\pm$ 0.04 -0.39 $\pm$ 0.10 0.39 $\pm$ 0.08 0.32 $\pm$ 0.08 0.54 $\pm$ 0.10 0.47 $\pm$ 0.08 0.2 $\pm$ 0.1
Cc 0.08 $\pm$ 0.02 14.76 $\pm$ 0.04 -19.93 $\pm$ 0.04 -0.52 $\pm$ 0.08 0.29 $\pm$ 0.08 0.31 $\pm$ 0.08 0.25 $\pm$ 0.08 0.38 $\pm$ 0.08 0.22 $\pm$ 0.08
UC 0.11a ... ... -0.29 $\pm$ 0.10 0.44 $\pm$ 0.08 0.37 $\pm$ 0.08 0.98 $\pm$ 0.10 0.56 $\pm$ 0.14 0.22 $\pm$ 0.18

Mkn 1199c
0.15a 12.98 $\pm$ 0.03 -20.68 $\pm$ 0.03 -0.44 $\pm$ 0.06 0.46 $\pm$ 0.06 0.29 $\pm$ 0.06 1.30 $\pm$ 0.07 0.55 $\pm$ 0.08 0.34 $\pm$ 0.08
MB 0.21 $\pm$ 0.02 12.99 $\pm$ 0.04 -20.67 $\pm$ 0.04 -0.53 $\pm$ 0.08 0.41 $\pm$ 0.08 0.17 $\pm$ 0.08 1.12 $\pm$ 0.08 0.55 $\pm$ 0.08 0.33 $\pm$ 0.08
Center (C) 0.21 $\pm$ 0.02 13.56 $\pm$ 0.04 -20.10 $\pm$ 0.04 -0.63 $\pm$ 0.08 0.24 $\pm$ 0.08 0.15 $\pm$ 0.08 1.17 $\pm$ 0.08 0.44 $\pm$ 0.08 0.26 $\pm$ 0.08
NE 0.11 $\pm$ 0.02 16.09 $\pm$ 0.04 -17.57 $\pm$ 0.04 0.16 $\pm$ 0.08 0.51 $\pm$ 0.08 0.34 $\pm$ 0.08 1.29 $\pm$ 0.08 0.62 $\pm$ 0.10 0.20 $\pm$ 0.12
NE c 0.11 $\pm$ 0.02 18.12 $\pm$ 0.04 -15.54 $\pm$ 0.04 -0.45 $\pm$ 0.08 0.28 $\pm$ 0.08 0.25 $\pm$ 0.08 ... ... ...
e 0.12 $\pm$ 0.03d 18.99 $\pm$ 0.05 -14.67 $\pm$ 0.05 -0.50 $\pm$ 0.10 0.39 $\pm$ 0.10 0.15 $\pm$ 0.10 ... ... ...
UC 0.15a ... ... -0.12 $\pm$ 0.12 0.51 $\pm$ 0.08 0.31 $\pm$ 0.08 1.22 $\pm$ 0.12 0.65 $\pm$ 0.16 0.32 $\pm$ 0.18

Mkn 5
0.20 $\pm$ 0.02a 14.83 $\pm$ 0.03 -15.57 $\pm$ 0.03 -0.41 $\pm$ 0.06 0.44 $\pm$ 0.06 0.30 $\pm$ 0.06 0.81e 0.52 $\pm$ 0.03e 0.38 $\pm$ 0.04e
Main Body 0.20 $\pm$ 0.02a 15.46 $\pm$ 0.04 -14.94 $\pm$ 0.04 -0.57 $\pm$ 0.08 0.39 $\pm$ 0.08 0.21 $\pm$ 0.08 ... ... ...
Ac 0.18 $\pm$ 0.02 16.54 $\pm$ 0.04 -13.86 $\pm$ 0.04 -0.81 $\pm$ 0.08 0.10 $\pm$ 0.08 0.12 $\pm$ 0.08 ... ... ...
Bd 0.21 $\pm$ 0.02 19.13 $\pm$ 0.04 -11.27 $\pm$ 0.04 -0.48 $\pm$ 0.08 0.29 $\pm$ 0.08 0.09 $\pm$ 0.08 ... ... ...
c 0.20 $\pm$ 0.02a 20.14 $\pm$ 0.04 -10.26 $\pm$ 0.04 -0.17 $\pm$ 0.08 0.43 $\pm$ 0.08 0.27 $\pm$ 0.08 ... ... ...
UC 0.20 $\pm$ 0.02a ... ... ... 0.45 $\pm$ 0.08 0.30 $\pm$ 0.08 ... ... ...

IRAS 08208+2816c
0.17 $\pm$ 0.02a 15.10 $\pm$ 0.03 -21.29 $\pm$ 0.03 -0.49 $\pm$ 0.06 0.22 $\pm$ 0.06 0.35 $\pm$ 0.08 1.03 $\pm$ 0.08 0.54 $\pm$ 0.08 0.22 $\pm$ 0.10
#1c 0.30 $\pm$ 0.03 19.15 $\pm$ 0.04 -17.24 $\pm$ 0.04 -0.52 $\pm$ 0.08 0.19 $\pm$ 0.06 0.30 $\pm$ 0.12 ... ... ...
#2c 0.30 $\pm$ 0.03 19.22 $\pm$ 0.05 -17.17 $\pm$ 0.05 -0.55 $\pm$ 0.08 0.19 $\pm$ 0.06 0.19 $\pm$ 0.12 ... ... ...
#3c 0.33 $\pm$ 0.02 16.80 $\pm$ 0.03 -19.59 $\pm$ 0.03 -0.50 $\pm$ 0.08 0.05 $\pm$ 0.06 0.05 $\pm$ 0.12 0.80 $\pm$ 0.12 0.51 $\pm$ 0.14 0.26 $\pm$ 0.16
#5c 0.28 $\pm$ 0.02 17.83 $\pm$ 0.03 -18.56 $\pm$ 0.03 -0.65 $\pm$ 0.08 0.07 $\pm$ 0.06 0.08 $\pm$ 0.12 ... ... ...
#6(C)c 0.08 $\pm$ 0.02 16.91 $\pm$ 0.03 -19.48 $\pm$ 0.03 -0.61 $\pm$ 0.06 0.02 $\pm$ 0.06 0.24 $\pm$ 0.08 0.57 $\pm$ 0.10 0.27 $\pm$ 0.08 0.18 $\pm$ 0.10
#7c 0.10 $\pm$ 0.02 20.60 $\pm$ 0.03 -15.79 $\pm$ 0.03 -0.44 $\pm$ 0.06 0.37 $\pm$ 0.06 0.39 $\pm$ 0.08 ... ... ...
#8c 0.12 $\pm$ 0.02 17.84 $\pm$ 0.03 -18.55 $\pm$ 0.03 -0.31 $\pm$ 0.06 0.30 $\pm$ 0.06 0.31 $\pm$ 0.08 1.05 $\pm$ 0.12 0.53 $\pm$ 0.12 0.28 $\pm$ 0.14
#9c 0.10 $\pm$ 0.02 18.42 $\pm$ 0.05 -17.97 $\pm$ 0.05 -0.20 $\pm$ 0.06 0.32 $\pm$ 0.06 0.32 $\pm$ 0.08 ... ... ...
#10c 0.08 $\pm$ 0.02 18.04 $\pm$ 0.04 -18.35 $\pm$ 0.04 -0.20 $\pm$ 0.06 0.29 $\pm$ 0.06 0.35 $\pm$ 0.08 ... ... ...

IRAS 08339+6517c,d
0.16 $\pm$ 0.02 12.94 $\pm$ 0.04 -21.57 $\pm$ 0.04 -0.51 $\pm$ 0.08 0.01 $\pm$ 0.08 0.26 $\pm$ 0.08 1.36 $\pm$ 0.06e 0.64 $\pm$ 0.05e 0.23 $\pm$ 0.06e
Companiond 0.13 $\pm$ 0.02 16.31 $\pm$ 0.04 -18.21 $\pm$ 0.04 -0.16 $\pm$ 0.10 0.20 $\pm$ 0.08 0.26 $\pm$ 0.08 1.45 $\pm$ 0.12e 0.21 $\pm$ 0.25e 0.68 $\pm$ 0.28e
POX 4c 0.06d 14.56 $\pm$ 0.01 -18.79 $\pm$ 0.01 -0.68 $\pm$ 0.03 0.29 $\pm$ 0.02 0.32 $\pm$ 0.04 0.42 $\pm$ 0.08 0.28 $\pm$ 0.08 0.15 $\pm$ 0.10
#3c 0.06d 17.88 $\pm$ 0.01 -15.41 $\pm$ 0.01 -1.00 $\pm$ 0.03 -0.06 $\pm$ 0.02 0.04 $\pm$ 0.04 0.12 $\pm$ 0.10 ... ...
#6c 0.06d 18.49 $\pm$ 0.02 -14.80 $\pm$ 0.02 -0.98 $\pm$ 0.04 -0.01 $\pm$ 0.04 0.06 $\pm$ 0.06 0.08 $\pm$ 0.12 ... ...
#7c 0.06d 20.69 $\pm$ 0.02 -12.60 $\pm$ 0.02 -0.88 $\pm$ 0.04 -0.09 $\pm$ 0.06 0.11 $\pm$ 0.08 ... ... ...
#9 (C)c 0.06 $\pm$ 0.02 15.32 $\pm$ 0.01 -17.97 $\pm$ 0.01 -0.93 $\pm$ 0.03 0.32 $\pm$ 0.02 0.10 $\pm$ 0.04 0.16 $\pm$ 0.12 0.2: 0.2:
#11c 0.06d 19.19 $\pm$ 0.04 -14.10 $\pm$ 0.04 -0.65 $\pm$ 0.06 0.07 $\pm$ 0.02 0.15 $\pm$ 0.04 0.49 $\pm$ 0.14 ... ...
Comp 0.12 17.93 $\pm$ 0.03 -15.36 $\pm$ 0.03 -0.02 $\pm$ 0.06 0.25 $\pm$ 0.02 0.30 $\pm$ 0.04 0.87 $\pm$ 0.10 0.7: 0.3:

UM 420
0.06 $\pm$ 0.01 17.32 $\pm$ 0.03 -19.55 $\pm$ 0.03 -0.80 $\pm$ 0.06 0.31 $\pm$ 0.06 0.13 $\pm$ 0.06d 0.77 $\pm$ 0.12 0.41 $\pm$ 0.12 0.12 $\pm$ 0.16
Cc 0.06 $\pm$ 0.01 19.35 $\pm$ 0.03 -17.52 $\pm$ 0.03 -1.00 $\pm$ 0.06 0.11 $\pm$ 0.06 0.18 $\pm$ 0.06 0.38 $\pm$ 0.12 0.32 $\pm$ 0.12 0.13 $\pm$ 0.16
UGC 1809 0.04b 15.02 $\pm$ 0.03 -19.92 $\pm$ 0.03e 0.12 $\pm$ 0.06 0.49 $\pm$ 0.06 0.50 $\pm$ 0.06 1.40 $\pm$ 0.10 0.68 $\pm$ 0.12 0.28 $\pm$ 0.14

SBS 0926+606 Ac
0.08 $\pm$ 0.02 16.45 $\pm$ 0.03 -17.29 $\pm$ 0.03 -0.75 $\pm$ 0.06 0.01 $\pm$ 0.06 0.14 $\pm$ 0.06 0.54 $\pm$ 0.06 0.21 $\pm$ 0.06 0.15 $\pm$ 0.08
A1c 0.08 $\pm$ 0.02 17.51 $\pm$ 0.03 -16.23 $\pm$ 0.03 -0.77 $\pm$ 0.06 -0.02 $\pm$ 0.06 0.10 $\pm$ 0.06 0.34 $\pm$ 0.08 0.18 $\pm$ 0.08 0.11 $\pm$ 0.08
A2c 0.08 $\pm$ 0.02 17.92 $\pm$ 0.03 -15.82 $\pm$ 0.03 -0.84 $\pm$ 0.06 -0.05 $\pm$ 0.06 0.08 $\pm$ 0.06 0.29 $\pm$ 0.08 0.18 $\pm$ 0.08 0.12 $\pm$ 0.08
AUC 0.08 $\pm$ 0.02 19.15 $\pm$ 0.04 -14.59 $\pm$ 0.04 -0.20 $\pm$ 0.10 0.25 $\pm$ 0.08 0.32 $\pm$ 0.08 0.98 $\pm$ 0.10 0.57 $\pm$ 0.10 0.16 $\pm$ 0.12

SBS 0926+606 Bc
0.12 $\pm$ 0.02 16.37 $\pm$ 0.04 -17.37 $\pm$ 0.04 -0.51 $\pm$ 0.08 0.08 $\pm$ 0.06 0.20 $\pm$ 0.06 0.83 $\pm$ 0.06 0.29 $\pm$ 0.06 0.18 $\pm$ 0.08
Bcc 0.12 $\pm$ 0.02 18.84 $\pm$ 0.04 -14.90 $\pm$ 0.04 -0.87 $\pm$ 0.08 0.04 $\pm$ 0.06 0.11 $\pm$ 0.06 0.52 $\pm$ 0.12 ... ...
BMBc 0.12 $\pm$ 0.02 17.21 $\pm$ 0.03 -16.53 $\pm$ 0.03 -0.54 $\pm$ 0.06 0.13 $\pm$ 0.06 0.16 $\pm$ 0.06 0.75 $\pm$ 0.06 0.20 $\pm$ 0.06 0.16 $\pm$ 0.08
Bdc 0.12 $\pm$ 0.02 21.60 $\pm$ 0.12 -12.14 $\pm$ 0.12 -0.58 $\pm$ 0.20 0.06 $\pm$ 0.12 0.10 $\pm$ 0.08 0.80 $\pm$ 0.20 ... ...
BUC 0.12 $\pm$ 0.02 16.69 $\pm$ 0.04 -17.05 $\pm$ 0.04 -0.33 $\pm$ 0.10 0.30 $\pm$ 0.08 0.29 $\pm$ 0.08 1.10 $\pm$ 0.10 0.53 $\pm$ 0.10 0.13 $\pm$ 0.12

X
0.03b 24.4:d ... ... 2.4: 1.4 $\pm$ 0.2 4.4 $\pm$ 0.2 1.07 $\pm$ 0.14 0.65 $\pm$ 0.18

SBS 0948+532c
0.24 $\pm$ 0.02 17.93 $\pm$ 0.03 -18.43 $\pm$ 0.03 -1.20 $\pm$ 0.06 -0.12 $\pm$ 0.06 0.16 $\pm$ 0.06 ... ... ...
r=1.3 $\hbox{$^{\prime\prime}$ }$c 0.24 $\pm$ 0.02 18.19 $\pm$ 0.03 -18.17 $\pm$ 0.03 -0.90 $\pm$ 0.06 -0.03 $\pm$ 0.06 0.07 $\pm$ 0.06 ... ... ...
r=2.3 $\hbox{$^{\prime\prime}$ }$c 0.24 $\pm$ 0.02 17.89 $\pm$ 0.03 -18.47 $\pm$ 0.03 -1.19 $\pm$ 0.06 -0.05 $\pm$ 0.06 0.15 $\pm$ 0.06 ... ... ...
Tail 0.24 $\pm$ 0.02 20.59 $\pm$ 0.05 -15.77 $\pm$ 0.05 -0.40 $\pm$ 0.20 0.28 $\pm$ 0.09 0.30 $\pm$ 0.06 ... ... ...

SBS 1054+365
0.02d 15.46 $\pm$ 0.03 -14.06 $\pm$ 0.03 -0.34 $\pm$ 0.06 0.33 $\pm$ 0.06 ... 0.92 $\pm$ 0.08 0.38 $\pm$ 0.12 0.16 $\pm$ 0.15
Main Bodye 0.02d 15.83 $\pm$ 0.03 -13.69 $\pm$ 0.03 -0.45 $\pm$ 0.06 0.23 $\pm$ 0.06 ... 0.72 $\pm$ 0.08 ... ...
Cc 0.02d 17.81 $\pm$ 0.03 -11.71 $\pm$ 0.03 -0.69 $\pm$ 0.06 -0.02 $\pm$ 0.06 ... 0.22 $\pm$ 0.10 0.20: 0.14:
ae 0.02d 18.81 $\pm$ 0.03 -10.71 $\pm$ 0.03 -0.52 $\pm$ 0.06 0.19 $\pm$ 0.06 ... 0.50 $\pm$ 0.12 ... ...
bc 0.02d 18.47 $\pm$ 0.03 -11.05 $\pm$ 0.03 -0.52 $\pm$ 0.06 0.16 $\pm$ 0.06 ... 0.79 $\pm$ 0.12 0.15: 0.10:
d 0.02d 19.97 $\pm$ 0.03 -9.55 $\pm$ 0.03 -0.55 $\pm$ 0.06 0.10 $\pm$ 0.06 ... 0.70 $\pm$ 0.12 ... ...
UC 0.02d ... ... 0.11 $\pm$ 0.08 0.42 $\pm$ 0.08 ... 1.05 $\pm$ 0.15 0.7: ...

Comp
0.02d 16.84 $\pm$ 0.03 ... -0.10 $\pm$ 0.06 0.61 $\pm$ 0.06 ... ... ... ...
Comp Cf 0.02d 17.42 $\pm$ 0.03 ... -0.28 $\pm$ 0.06 0.49 $\pm$ 0.06 ... 1.75 $\pm$ 0.08 0.66 $\pm$ 0.10 0.27 $\pm$ 0.15

SBS 1211+540c
0.08 $\pm$ 0.01 17.32 $\pm$ 0.03 -13.27 $\pm$ 0.03 -0.61 $\pm$ 0.06 0.04 $\pm$ 0.06 0.21 $\pm$ 0.06 ... ... ...
Cc 0.08 $\pm$ 0.01 18.67 $\pm$ 0.03 -11.92 $\pm$ 0.03 -0.89 $\pm$ 0.06 -0.03 $\pm$ 0.06 0.13 $\pm$ 0.06 ... ... ...
ac 0.08 $\pm$ 0.01 20.53 $\pm$ 0.03 -10.06 $\pm$ 0.03 -0.71 $\pm$ 0.06 0.00 $\pm$ 0.06 0.15 $\pm$ 0.06 ... ... ...
b 0.08 $\pm$ 0.01 22.4 $\pm$ 0.1 -8.2 $\pm$ 0.1 ... 0.45 $\pm$ 0.15 0.48 $\pm$ 0.10 ... ... ...
UC 0.08 $\pm$ 0.01 ... ... -0.21 $\pm$ 0.06 0.29 $\pm$ 0.06 0.35 $\pm$ 0.06 ... ... ...

SBS 1319+579
0.02 $\pm$ 0.01 15.32 $\pm$ 0.03 -18.53 $\pm$ 0.03 -0.39 $\pm$ 0.06 0.34 $\pm$ 0.06 0.19 $\pm$ 0.06 1.03 $\pm$ 0.08 0.39 $\pm$ 0.12 0.16 $\pm$ 0.20
Ac 0.02 $\pm$ 0.01 17.61 $\pm$ 0.03 -16.24 $\pm$ 0.03 -0.77 $\pm$ 0.06 -0.04 $\pm$ 0.06 0.02 $\pm$ 0.06 0.31 $\pm$ 0.12 0.21 $\pm$ 0.14 0.15 $\pm$ 0.20
Bc 0.08 $\pm$ 0.02 17.41 $\pm$ 0.03 -16.44 $\pm$ 0.03 -0.45 $\pm$ 0.08 0.12 $\pm$ 0.06 0.25 $\pm$ 0.06 0.88 $\pm$ 0.12 0.28 $\pm$ 0.16 ...
Cc 0.02 $\pm$ 0.01 17.98 $\pm$ 0.03 -15.87 $\pm$ 0.03 -0.72 $\pm$ 0.06 0.02 $\pm$ 0.06 0.12 $\pm$ 0.06 0.68 $\pm$ 0.12 0.25 $\pm$ 0.16 0.20:
UC 0.02 $\pm$ 0.01 ... ... -0.15 $\pm$ 0.08 0.29 $\pm$ 0.06 0.33 $\pm$ 0.06 1.20 $\pm$ 0.20 ... ...

SBS 1415+437
0.13 $\pm$ 0.02 15.32 $\pm$ 0.03 -14.52 $\pm$ 0.03 -0.47 $\pm$ 0.06 0.21 $\pm$ 0.06 0.27 $\pm$ 0.06 0.98 $\pm$ 0.08 0.35 $\pm$ 0.10 0.15:
C 0.13 $\pm$ 0.02 16.97 $\pm$ 0.03 -12.87 $\pm$ 0.03 -0.75 $\pm$ 0.06 0.01 $\pm$ 0.06 0.08 $\pm$ 0.06 0.60 $\pm$ 0.12 0.20 $\pm$ 0.14 0.1:
a 0.13 $\pm$ 0.02 19.04 $\pm$ 0.03 -10.80 $\pm$ 0.03 -0.68 $\pm$ 0.06 0.06 $\pm$ 0.06 0.12 $\pm$ 0.06 ... ... ...
b 0.13 $\pm$ 0.02 19.53 $\pm$ 0.03 -10.31 $\pm$ 0.03 -0.49 $\pm$ 0.06 0.18 $\pm$ 0.06 0.31 $\pm$ 0.06 ... ... ...
UC 0.13 $\pm$ 0.02 ... - ... -0.17 $\pm$ 0.08 0.27 $\pm$ 0.06 0.38 $\pm$ 0.06 1.10 $\pm$ 0.14 ... ...

bg
0.009b 19.69 $\pm$ 0.03 ... 0.33 $\pm$ 0.08 1.35 $\pm$ 0.06 0.88 $\pm$ 0.06 1.22 $\pm$ 0.12 0.55 $\pm$ 0.14 ...
III Zw 107c 0.21 $\pm$ 0.02 14.36 $\pm$ 0.03 -20.14 $\pm$ 0.03 -0.42 $\pm$ 0.06 0.14 $\pm$ 0.06 0.22 $\pm$ 0.06 0.62 $\pm$ 0.12 0.47 $\pm$ 0.20 0.35 $\pm$ 0.20
Ac,d 0.47 $\pm$ 0.02 15.67 $\pm$ 0.03 -18.83 $\pm$ 0.03 -0.68 $\pm$ 0.06 -0.01 $\pm$ 0.06 0.15 $\pm$ 0.06 0.56 $\pm$ 0.12 0.36 $\pm$ 0.20 0.20 $\pm$ 0.20
B+Cc,d 0.11 $\pm$ 0.02 15.75 $\pm$ 0.03 -18.75 $\pm$ 0.03 -0.57 $\pm$ 0.06 0.02 $\pm$ 0.06 0.18 $\pm$ 0.06 0.76 $\pm$ 0.14 0.42 $\pm$ 0.20 0.24 $\pm$ 0.20
Tail 0.21 $\pm$ 0.02 18.66 $\pm$ 0.03 -15.84 $\pm$ 0.03 -0.15 $\pm$ 0.06 0.20 $\pm$ 0.06 0.30 $\pm$ 0.06 ... ... ...
UC 0.21 $\pm$ 0.02 ... ... 0.06 $\pm$ 0.10 0.40 $\pm$ 0.08 0.30 $\pm$ 0.08 1.2: ... ...

Tol 9c
0.31 $\pm$ 0.03 13.92 $\pm$ 0.03 -19.26 $\pm$ 0.03 -0.34 $\pm$ 0.06 0.24 $\pm$ 0.06 0.22 $\pm$ 0.06 0.83 $\pm$ 0.08 0.68 $\pm$ 0.10 0.27 $\pm$ 0.12
UC 0.31 $\pm$ 0.03 ... ... 0.04 $\pm$ 0.10 0.48 $\pm$ 0.08 0.33 $\pm$ 0.08 1.10 $\pm$ 0.20 ... ...

Comp 1
0.07b 16.78 $\pm$ 0.03 -16.40 $\pm$ 0.03 0.17 $\pm$ 0.08 0.63 $\pm$ 0.06 0.39 $\pm$ 0.06 1.15 $\pm$ 0.10 0.69 $\pm$ 0.14 0.29 $\pm$ 0.16
Comp 2 0.07b 15.33 $\pm$ 0.03 -17.85 $\pm$ 0.03 0.29 $\pm$ 0.06 0.65 $\pm$ 0.06 0.52 $\pm$ 0.06 1.55 $\pm$ 0.10 0.73 $\pm$ 0.14 0.30 $\pm$ 0.16

Tol 1457-262
                 
Obj 1c 0.16b 14.44 $\pm$ 0.03 -19.73 $\pm$ 0.03 -0.56 $\pm$ 0.06 0.23 $\pm$ 0.06 0.26 $\pm$ 0.06 0.60 $\pm$ 0.10 0.51 $\pm$ 0.12 0.22 $\pm$ 0.12
Ac 0.57 14.47 $\pm$ 0.03 -19.70 $\pm$ 0.03 -0.80 $\pm$ 0.06 0.08 $\pm$ 0.06 0.11 $\pm$ 0.06 0.30 $\pm$ 0.12 0.38 $\pm$ 0.12 0.15 $\pm$ 0.12
Bc 0.16b 16.31 $\pm$ 0.03 -17.86 $\pm$ 0.03 -0.63 $\pm$ 0.06 0.13 $\pm$ 0.06 0.16 $\pm$ 0.06 0.40 $\pm$ 0.12 0.35 $\pm$ 0.12 0.19 $\pm$ 0.14
Cc 0.16b 17.63 $\pm$ 0.03 -16.54 $\pm$ 0.03 -0.58 $\pm$ 0.06 0.26 $\pm$ 0.06 0.21 $\pm$ 0.06 ... ... ...
dc 0.16b 17.21 $\pm$ 0.03 -16.96 $\pm$ 0.03 -0.49 $\pm$ 0.06 0.19 $\pm$ 0.06 0.11 $\pm$ 0.06 0.60 $\pm$ 0.16 ... ...
UC 0.16b ... ... -0.30 $\pm$ 0.14 0.31 $\pm$ 0.12 0.32 $\pm$ 0.08 1.20 $\pm$ 0.20 ... ...

Obj 2c
0.16b 15.20 $\pm$ 0.03 -18.97 $\pm$ 0.03 -0.42 $\pm$ 0.06 0.34 $\pm$ 0.06 0.36 $\pm$ 0.06 0.90 $\pm$ 0.10 0.58 $\pm$ 0.12 0.27 $\pm$ 0.14
ec 0.16b 17.17 $\pm$ 0.03 -17.00 $\pm$ 0.03 -0.61 $\pm$ 0.06 0.27 $\pm$ 0.06 0.36 $\pm$ 0.06 1.10 $\pm$ 0.20 ... ...
fc 0.16b 16.81 $\pm$ 0.03 -17.36 $\pm$ 0.03 -0.53 $\pm$ 0.06 0.37 $\pm$ 0.06 0.33 $\pm$ 0.06 1.30 $\pm$ 0.20 ... ...
gc 0.16b 15.93 $\pm$ 0.03 -18.24 $\pm$ 0.03 -0.30 $\pm$ 0.06 0.44 $\pm$ 0.06 0.41 $\pm$ 0.06 1.20 $\pm$ 0.20 ... ...
UC 0.16b ... ... -0.17 $\pm$ 0.14 0.45 $\pm$ 0.12 0.53 $\pm$ 0.08 1.30 $\pm$ 0.20 ... ...

#15
0.16b 17.69 $\pm$ 0.04 -16.48 $\pm$ 0.04 -0.25 $\pm$ 0.10 0.39 $\pm$ 0.08 0.39 $\pm$ 0.06 1.10 $\pm$ 0.20 ... ...
#16 0.16b 19.48 $\pm$ 0.05 -14.69 $\pm$ 0.05 -0.10 $\pm$ 0.15 0.45 $\pm$ 0.10 0.40 $\pm$ 0.06 ... ... ...

Arp 252d
                 

A
0.34 $\pm$ 0.02 14.69 $\pm$ 0.03 -20.88 $\pm$ 0.03 -0.48 $\pm$ 0.06 0.31 $\pm$ 0.06 0.19 $\pm$ 0.06 1.10 $\pm$ 0.10 0.60 $\pm$ 0.12 0.38 $\pm$ 0.14e
Aa1c 0.34 $\pm$ 0.02 15.27 $\pm$ 0.03 -20.30 $\pm$ 0.03 -0.67 $\pm$ 0.06 0.08 $\pm$ 0.06 0.14 $\pm$ 0.06 0.95 $\pm$ 0.10 0.48 $\pm$ 0.12 ...
Aa2 0.34 $\pm$ 0.02 17.77 $\pm$ 0.03 -17.80 $\pm$ 0.03 -0.50 $\pm$ 0.06 0.12 $\pm$ 0.06 0.17 $\pm$ 0.06 1.10 $\pm$ 0.20 ... ...
c 0.34 $\pm$ 0.02 19.89 $\pm$ 0.04 -15.58 $\pm$ 0.04 -0.75 $\pm$ 0.09 0.03 $\pm$ 0.07 0.08 $\pm$ 0.06 ... ... ...
At 0.34 $\pm$ 0.02 ... ... ... 0.26 $\pm$ 0.08 0.24 $\pm$ 0.07 ... ... ...
B 0.16 $\pm$ 0.03 16.22 $\pm$ 0.03 -19.35 $\pm$ 0.03 -0.21 $\pm$ 0.08 0.49 $\pm$ 0.06 0.31 $\pm$ 0.06 1.20 $\pm$ 0.10 0.71 $\pm$ 0.16 0.34 $\pm$ 0.20e
Bcenc 0.16 $\pm$ 0.03 16.51 $\pm$ 0.03 -19.06 $\pm$ 0.03 -0.41 $\pm$ 0.06 0.38 $\pm$ 0.06 0.30 $\pm$ 0.06 1.00 $\pm$ 0.10 0.52 $\pm$ 0.12 ...
d 0.16 $\pm$ 0.03 21.65 $\pm$ 0.05 -13.92 $\pm$ 0.05 -0.35 $\pm$ 0.12 0.23 $\pm$ 0.10 0.10 $\pm$ 0.08 ... ... ...
e 0.16 $\pm$ 0.03 19.45 $\pm$ 0.04 -16.12 $\pm$ 0.04 -0.31 $\pm$ 0.09 0.27 $\pm$ 0.07 0.20 $\pm$ 0.06 ... ... ...
BtN 0.16 $\pm$ 0.03 17.22 $\pm$ 0.04 -18.35 $\pm$ 0.04 0.05 $\pm$ 0.10 0.43 $\pm$ 0.08 0.29 $\pm$ 0.06 1.30 $\pm$ 0.20 ... ...
BtS 0.16 $\pm$ 0.03 ... ... 0.20 $\pm$ 0.12 0.53 $\pm$ 0.08 0.39 $\pm$ 0.06 ... ... ...

NGC 5253c,d
0.17 $\pm$ 0.03 10.09 $\pm$ 0.01 -17.92 $\pm$ 0.01 -0.41 $\pm$ 0.02 0.27 $\pm$ 0.02 0.21 $\pm$ 0.02 0.81 $\pm$ 0.03 0.53 $\pm$ 0.04 0.19 $\pm$ 0.05
Notes for Table 5:
a Average value of the E(B-V) obtained in objects/regions inside the galaxy.
b Using the value for the Galactic extinction given by Schlegel et al. (1998).
c The optical colors of this object have been corrected for the emission of the ionized gas, consult Table 6.
d Notes 1: HCG 31 See results in López-Sánchez et al. (2004a), member AC is NGC 1741. Mkn 1087: see results in López-Sánchez et al. (2004b). Haro 15: using Cairós et al. (2001a) data. Mkn 1199: assuming a value similar to the near region B, that has not been analyzed by photometry but by spectroscopy. Mkn 5: the colors of this object should be also corrected for emission of the gas, but as we do not have spectroscopic data it was not done. B-V should be slightly lower and V-R slightly higher. IRAS 08339+6517: results extracted from López-Sánchez et al. (2006). POX 4: using the E(B-V) derived for the central object. UM 420: The H$\alpha $ emission in this object is very important; correcting for our H$\alpha $ flux $(V-R)\sim 0.25$. SBS 0926+606 X: the B-magnitude of this object is very uncertain. Its V and $K_{\rm s}$ magnitudes are mV = 22.1 $\pm$ 0.1 and $m_{K_{\rm s}}=15.91$ $\pm$ 0.12, hence it possesses $V-K_{\rm s}\sim6.2$. SBS 0948+532: using the values given by 2MASS, mJ=16.86, mH=15.92 and $m_{K_{\rm s}}=15.31$. SBS 1054+365: because of the C(H$\beta $) derived from our spectrum gives E(B-V)=0.01, we use the Galactic value, E(B-V)G = 0.02 (Schlegel et al. 1998). III Zw 107: using the data for J, H and $K_{\rm s}$ provided by 2MASS. Arp 252: object A is ESO 566-8 and object B ESO 566-7. NGC 5253: optical and NIR magnitudes extracted from the NED and corrected for extinction using an average value of C(H$\beta $) = 0.24 (see López-Sánchez et al. 2007).
e NOTES 2: Mkn 5: using the data provided by Noeske et al. (2005), who used K' instead of $K_{\rm s}$ filter. For the low-brightness underlying stellar component, they found J-H=0.58 y H-K'=0.28. IRAS 08339+6517: NIR values extracted from 2MASS, see López-Sánchez et al. (2006). UM 420 / UGC 1809: calculated using $V_{\rm r}=7306$ km s-1 (given by the NED) and its derived distance, D=97.4 Mpc. SBS 1054+365: probably, the colors have a small contribution for the nebular component. Arp 252: $H-K_{\rm s}$ color adapted from 2MASS.
f NOTES 3: SBS 1054+365: Comp C is the central region of the companion object, 2MASX J10574661+3616582.


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