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Table 4:

SDSS photometry of LGG 225 members.

Galaxy
u g r i z
  [AB mag] [AB mag] [AB mag] [AB mag] [AB mag]
NGC 3370 13.31 $\pm $ 0.06 12.31 $\pm $ 0.02 11.85 $\pm $ 0.03 11.59 $\pm $ 0.03 11.38 $\pm $ 0.06
NGC 3443b 15.91 $\pm $ 0.14 14.79 $\pm $ 0.05 14.33 $\pm $ 0.05 14.11 $\pm $ 0.06 13.90 $\pm $ 0.18
NGC 3447b 14.47 $\pm $ 0.12 13.22 $\pm $ 0.04 12.90 $\pm $ 0.05 12.78 $\pm $ 0.06 12.06 $\pm $ 0.10
NGC 3447A 15.34 $\pm $ 0.16 14.89 $\pm $ 0.09 14.71 $\pm $ 0.13 14.65 $\pm $ 0.19 14.32 $\pm $ 0.44
NGC 3454 15.08 $\pm $ 0.12 13.84 $\pm $ 0.03 13.23 $\pm $ 0.03 12.91 $\pm $ 0.04 12.66 $\pm $ 0.09
NGC 3455 13.98 $\pm $ 0.09 13.02 $\pm $ 0.03 12.66 $\pm $ 0.04 12.50 $\pm $ 0.05 12.31 $\pm $ 0.12
NGC 3457 14.69 $\pm $ 0.06 13.05 $\pm $ 0.02 12.37 $\pm $ 0.02 12.01 $\pm $ 0.02 11.77 $\pm $ 0.04
NGC 3501 14.41 $\pm $ 0.07 13.06 $\pm $ 0.02 12.40 $\pm $ 0.02 11.99 $\pm $ 0.03 11.68 $\pm $ 0.05
NGC 3507a,b 12.16 $\pm $ 0.02 10.75 $\pm $ 0.02 10.18 $\pm $ 0.02 9.78 $\pm $ 0.02 9.62 $\pm $ 0.03
NGC 3522 15.16 $\pm $ 0.11 13.59 $\pm $ 0.03 12.88 $\pm $ 0.02 12.52 $\pm $ 0.03 12.37 $\pm $ 0.06
UGC 6022 16.94 $\pm $ 0.35 15.84 $\pm $ 0.11 15.52 $\pm $ 0.14 15.38 $\pm $ 0.19 15.07 $\pm $ 0.51
UGC 6035a 13.77 $\pm $ 0.11 12.90 $\pm $ 0.04 12.21 $\pm $ 0.06 11.75 $\pm $ 0.05 10.92 $\pm $ 0.13
UGC 6083 16.31 $\pm $ 0.17 15.17 $\pm $ 0.05 14.71 $\pm $ 0.06 14.43 $\pm $ 0.07 14.35 $\pm $ 0.23
UGC 6112b 15.22 $\pm $ 0.14 14.29 $\pm $ 0.05 13.94 $\pm $ 0.06 13.76 $\pm $ 0.08 13.75 $\pm $ 0.31
UGC 6171a 15.50 $\pm $ 0.15 13.41 $\pm $ 0.05 13.03 $\pm $ 0.06 12.79 $\pm $ 0.06 12.69 $\pm $ 0.14

Notes. (a) Magnitude of the foreground stars have been subtracted; (b) Galaxy is near SDSS edge, magnitudes have been computed in a reduced area (elliptical aperture with $a=0.5\hbox{$^\prime$ }$, $b=0.3\hbox{$^\prime$ }$for NGC 3443, with $a=1.6\hbox{$^\prime$ }$, $b=0.8\hbox{$^\prime$ }$for NGC 3447, with $a=1\hbox{$^\prime$ }$, $b=0.4\hbox{$^\prime$ }$for UGC 6112 and aperture of radius 0.9$^\prime$ for NGC 3507 respectively, and scaled to the total area using the UV ratio to derive their mass.


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