Table 6: Correction for the contribution of the nebular emission in optical colors. Corrections have been done applying $(X-Y)_{\rm e}=(X-Y)-\Delta (X-Y)$, being (X-Y) the color derived from photometry, $(X-Y)_{\rm e}$ the color corrected for emission lines and $\Delta (X-Y)$ the correction given in this table.

Object
$\Delta(U-B)$ $\Delta(B-V)$ $\Delta(V-R)$ $\Delta(V-J)$

HCG 31 AC
-0.040.12-0.070.04
HCG 31 B -0.010.03-0.010.04
HCG 31 E -0.050.07-0.030.03
HCG 31 F -0.100.84-0.470.91
HCG 31 G -0.040.11-0.030.10

Mkn 1087 C
0.000.010.020.02
Mkn 1087 N -0.020.02-0.060.04

Haro 15 C
-0.030.030.000.04
Haro 15 ESE 0.040.78-0.670.88
Haro 15 NE -0.020.03-0.010.03

Mkn 1199 C
0.000.00-0.070.01

Mkn 5 A
-0.030.29-0.180.40

IRAS 08208+2816
-0.010.20-0.100.20
#1, #2, #3, #5 -0.040.17-0.100.19
#6 (C) -0.010.52-0.470.62
#7, #8, #9, #10 -0.010.15-0.090.15

IRAS 08339+6517
0.000.01-0.020.03

POX 4a
-0.030.30-0.050.40

UM 420 C
-0.040.35-0.300.5

SBS 0926+606 A
-0.040.35-0.170.40
SBS 0926+606 B -0.030.08-0.060.10

SBS 0948+532
-0.02$\sim $0.7$\sim $-0.6...

SBS 1054+365 C
-0.140.45...0.47
SBS 1054+365 d 0.000.05......

SBS 1211+540 C
-0.190.47-0.40...
SBS 1211+540 ab -0.080.24-0.20...

SBS 1319+579 A
-0.05$\sim $0.7$\sim $-0.6$\sim $0.7
SBS 1319+579 B -0.010.12-0.120.19
SBS 1319+579 C -0.030.16-0.140.37

SBS 1415+437 C
-0.060.350.060.65

III Zw 107 A
-0.030.19-0.080.23
III Zw 107 B+C -0.030.03-0.010.03

Tol 9
-0.050.070.000.10

Tol 1457-262c
-0.05$\sim $0.5$\sim $-0.4$\sim $0.6
Tol 1457-262 A -0.02$\sim $0.2$\sim $-0.2$\sim $0.3

Arp 252 Aa1
-0.040.24-0.010.32
Arp 252 Bcen -0.010.01-0.030.01

NGC 5253
-0.020.06-0.020.04
a Because of the strong nebular emission in this object, all regions but the companion object have been corrected using these values; b these values have been also used to correct the colors of SBS 1211+540 integrating all its flux; c all objects (Obj 1, B, C, d, Obj 2, e, f and g) except region A.

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