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Table 3:

The GALEX photometry.

Group
FUV NUV (FUV - NUV)
galaxy [AB mag] [AB mag] [AB mag]
LGG 93      
NGC 1249 14.10 $\pm $ 0.07 13.66 $\pm $ 0.04 0.44 $\pm $ 0.09
NGC 1311 15.10 $\pm $ 0.08 14.68 $\pm $ 0.05 0.42 $\pm $ 0.10
IC 1933 14.34 $\pm $ 0.07 13.96 $\pm $ 0.04 0.39 $\pm $ 0.08
IC 1954 14.34 $\pm $ 0.07 13.87 $\pm $ 0.04 0.47 $\pm $ 0.08
IC 1959 14.74 $\pm $ 0.08 14.42 $\pm $ 0.05 0.32 $\pm $ 0.09
LGG 127      
NGC 1744 13.68 $\pm $ 0.07 13.31 $\pm $ 0.04 0.37 $\pm $ 0.08
NGC 1792 14.10 $\pm $ 0.07 13.31 $\pm $ 0.04 0.79 $\pm $ 0.08
NGC 1800 14.91 $\pm $ 0.08 14.56 $\pm $ 0.05 0.35 $\pm $ 0.09
NGC 1808 14.68 $\pm $ 0.08 13.94 $\pm $ 0.04 0.74 $\pm $ 0.09
NGC 1827 15.38 $\pm $ 0.09 14.58 $\pm $ 0.04 0.80 $\pm $ 0.10
ESO 305-009 14.97 $\pm $ 0.08 14.66 $\pm $ 0.05 0.31 $\pm $ 0.09
ESO 305-017 16.23 $\pm $ 0.09 15.91 $\pm $ 0.05 0.31 $\pm $ 0.11
ESO 362-011 15.14 $\pm $ 0.11 15.52 $\pm $ 0.04 0.62 $\pm $ 0.12
ESO 362-019 15.70 $\pm $ 0.21 15.39 $\pm $ 0.12 0.32 $\pm $ 0.25
LGG 225      
NGC 3370 14.65 $\pm $ 0.08 14.31 $\pm $ 0.04 0.34 $\pm $ 0.08
NGC 3443 15.85 $\pm $ 0.07 15.48 $\pm $ 0.04 0.37 $\pm $ 0.07
NGC 3447 14.82 $\pm $ 0.05 14.55 $\pm $ 0.03 0.27 $\pm $ 0.06
NGC 3447A 15.83 $\pm $ 0.06 15.72 $\pm $ 0.03 0.11 $\pm $ 0.06
NGC 3454 17.22 $\pm $ 0.07 16.60 $\pm $ 0.04 0.62 $\pm $ 0.08
NGC 3455 15.34 $\pm $ 0.06 14.77 $\pm $ 0.03 0.56 $\pm $ 0.06
NGC 3457 20.23 $\pm $ 0.13 17.76 $\pm $ 0.05 2.48 $\pm $ 0.14
NGC 3501 16.67 $\pm $ 0.09 16.12 $\pm $ 0.05 0.55 $\pm $ 0.11
NGC 3507a 14.55 $\pm $ 0.07 14.13 $\pm $ 0.04 0.42 $\pm $ 0.08
NGC 3522 19.92 $\pm $ 0.12 18.03 $\pm $ 0.05 1.90 $\pm $ 0.13
UGC 6022 17.82 $\pm $ 0.07 17.51 $\pm $ 0.04 0.31 $\pm $ 0.08
UGC 6035a 16.85 $\pm $ 0.06 16.52 $\pm $ 0.04 0.33 $\pm $ 0.07
UGC 6083 18.01 $\pm $ 0.13 17.48 $\pm $ 0.07 0.53 $\pm $ 0.15
UGC 6112 16.28 $\pm $ 0.09 15.85 $\pm $ 0.05 0.42 $\pm $ 0.10
UGC 6171a 16.41 $\pm $ 0.09 16.23 $\pm $ 0.05 0.18 $\pm $ 0.10

Notes. To avoid overlap in the elliptical apertures, coordinates and major and minor axes of NGC 3447A and NGC 3447 have been positioned as shown in Fig. 4.
(a) Magnitude of the foreground stars have been subtracted. Magnitudes are not corrected for galactic extinction.


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