Table 2: Results of optical and near-infrared aperture photometry in Mkn 1087 and KPG 103a knots.
Knot E(B-V) $m\rm _B$ $m\rm _B$0 $m\rm _J$0 (U-B)0 (B-V)0 (V-R)0 (V-J)0 (J-H)0 ( $H-K{\rm s}$)0
Mkn 1087 0.17a 13.78 13.08 $\pm$ 0.04 12.39 $\pm$ 0.04 -0.41 $\pm$ 0.08b 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
C 0.14 15.19 14.62 $\pm$ 0.03 14.33 $\pm$ 0.05 -0.57 $\pm$ 0.06b -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 0.10 17.58 17.17 $\pm$ 0.03 17.01 $\pm$ 0.06 ... -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 0.07c 19.18 18.89 $\pm$ 0.05 >18.7 -0.75 $\pm$ 0.15b -0.01 $\pm$ 0.08 0.10 $\pm$ 0.08 <0.2 ... ...
#2 0.07c 20.01 19.72 $\pm$ 0.05 >18.7 -0.78 $\pm$ 0.15b 0.05 $\pm$ 0.08 0.12 $\pm$ 0.08 <1 ... ...
#3 0.07c 18.32 18.03 $\pm$ 0.03 17.28 $\pm$ 0.06 0.08 $\pm$ 0.30b 0.11 $\pm$ 0.06 0.26 $\pm$ 0.06 0.64 $\pm$ 0.10 0.5 $\pm$ 0.2 ...
#7 0.16 18.29 17.63 $\pm$ 0.04 ... -0.87 $\pm$ 0.08b -0.04 $\pm$ 0.08 0.03 $\pm$ 0.08 ... ... ...
#8 0.08 19.10 18.77 $\pm$ 0.05 ... -0.27 $\pm$ 0.12b 0.07 $\pm$ 0.10 0.17 $\pm$ 0.08 ... ... ...
#11 0.07c 20.69 20.40 $\pm$ 0.05 ... ... 0.35 $\pm$ 0.10 0.08 $\pm$ 0.10 ... ... ...
#12 0.07c 19.61 19.32 $\pm$ 0.05 18.5 $\pm$ 0.1 -0.1 $\pm$ 0.3 0.31 $\pm$ 0.09 0.24 $\pm$ 0.08 0.55 $\pm$ 0.15 0.4 $\pm$ 0.2 ...
#13 0.40 19.25 17.61 $\pm$ 0.05 ... -0.64 $\pm$ 0.12 0.01 $\pm$ 0.09 0.04 $\pm$ 0.08 ... ... ...
#14 0.07 18.45 18.16 $\pm$ 0.05 ... -0.59 $\pm$ 0.12 0.28 $\pm$ 0.10 0.23 $\pm$ 0.10 ... ... ...
#15 0.19 20.90 20.12 $\pm$ 0.08 ... -0.6 $\pm$ 0.3 0.22 $\pm$ 0.12 0.23 $\pm$ 0.10 ... ... ...
KPG 103a 0.07c 14.05 13.77 $\pm$ 0.04 ... 0.17 $\pm$ 0.08b 0.18 $\pm$ 0.06 0.27 $\pm$ 0.06 ... ... ...
K1 0.07c 17.55 17.26 $\pm$ 0.05 ... -0.40 $\pm$ 0.10 0.18 $\pm$ 0.10 0.20 $\pm$ 0.08 ... ... ...
K2 0.07c 17.10 16.81 $\pm$ 0.04 ... -0.49 $\pm$ 0.08 0.12 $\pm$ 0.06 0.11 $\pm$ 0.06 ... ... ...
K3 0.07c 17.41 17.12 $\pm$ 0.04 ... -0.39 $\pm$ 0.08 0.19 $\pm$ 0.06 0.33 $\pm$ 0.06 ... ... ...
a Average of the values obtained for C, #7, #8, #13, #14 and #15.
b Adopting the mU values from ME00.
c Galactic reddening adopted from Schlegel et al. (1998), E(B-V) = 0.07.

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