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Table 4

Physical properties of the LSB galaxies assuming that they are satellites of the nearby (in projection) massive galaxies.

ID Re (pc) dP (kpc) Mr (mag)

NGC 3625-DGSAT-1 1145 ± 156 89.6 ± 9.8 − 13.0 ± 0.2 7.1 ± 0.1
NGC 3625-DGSAT-2 1536 ± 380 151.2 ± 16.6 − 12.8 ± 0.4 7.0 ± 0.2
NGC 3625-DGSAT-3 1480 ± 166 220.6 ± 24.2 − 14.1 ± 0.2 7.5 ± 0.1
NGC 3625-DGSAT-4 2175 ± 275 262.7 ± 28.9 − 14.5 ± 0.2 7.7 ± 0.1

NGC 3669-DGSAT-1 1064 ± 572 57.4 ± 30.6 − 12.7 ± 1.2 7.0 ± 0.5
NGC 3669-DGSAT-2 1864 ± 996 93.0 ± 49.5 − 13.1 ± 1.2 7.1 ± 0.5
NGC 3669-DGSAT-3 3912 ± 2094 123.1 ± 65.6 − 14.8 ± 1.2 7.8 ± 0.5
NGC 3669-DGSAT-4 1325 ± 709 196.6 ± 104.8 − 13.6 ± 1.2 7.3 ± 0.5

NGC 7814-DGSAT-1 1231 ± 269 15.6 ± 3.4 − 13.2 ± 0.5 7.2 ± 0.2
NGC 7814-DGSAT-2 2285 ± 504 46.7 ± 10.0 − 13.3 ± 0.5 7.2 ± 0.2
NGC 7814-DGSAT-3 901 ± 195 126.4 ± 27.1 − 12.9 ± 0.5 7.0 ± 0.2
NGC 7814-DGSAT-4 662 ± 147 129.8 ± 27.9 − 12.3 ± 0.5 6.8 ± 0.2
NGC 7814-DGSAT-5 366 ± 82 165.5 ± 35.5 − 10.4 ± 0.5 6.0 ± 0.2
NGC 7814-DGSAT-6 461 ± 100 187.6 ± 40.3 − 12.1 ± 0.5 6.7 ± 0.2
NGC 7814-DGSAT-7 1490 ± 360 257.9 ± 55.4 − 12.5 ± 0.5 6.9 ± 0.2

Notes. Re and dP are effective radius and projected distance of the dwarf candidate to the centre of the host galaxy, respectively. Mr denotes the absolute magnitude in r-band and the last column provides the logarithm of the r-band luminosity in units of solar luminosities, L.

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