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Table 2

Photometric and structural parameters of the new dwarf candidates in the surveyed region of the M 101 group complex.

Name g tot r tot M r (gr)0,tot μ 0,r r 0,r n r μeff,r r eff,r log reff,r
mag mag mag mag mag arcsec-2 arcsec mag arcsec-2 arcsec log  pc
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

M 101 subgroup
dw1343+58 15.54 15.17 14.0 0.370 18.93 ± 2.26 0.04 ± 0.77 0.27 ± 0.12 24.45 28.6 2.98
dw1355+51 18.76 18.09 11.1 0.666 23.09 ± 0.17 3.67 ± 0.69 0.78 ± 0.07 24.44 7.44 2.39
dw1408+56 18.01 17.50 11.7 0.507 23.28 ± 0.06 5.48 ± 0.38 0.89 ± 0.06 24.71 11.0 2.57
dw1412+56 19.46 18.75 10.5 0.702 24.26 ± 0.16 5.64 ± 0.80 1.22 ± 0.29 25.29 8.08 2.43
dw1416+57 19.06 18.83 10.4 0.227 24.86 ± 0.08 10.19 ± 0.47 2.16 ± 0.31 25.16 7.35 2.39
dw1446+58 18.46 17.90 11.3 0.559 23.87 ± 0.12 7.62 ± 0.74 1.27 ± 0.13 24.66 8.97 2.48
M 51 subgroup
dw1313+46 17.63 17.36 12.3 0.274 23.53 ± 0.04 9.33 ± 0.26 1.73 ± 0.07 23.78 7.69 2.50
dw1327+51 19.34 18.79 10.9 0.550 24.16 ± 0.09 6.36 ± 0.51 1.29 ± 0.15 24.74 6.19 2.41
dw1338+50 19.15 18.35 11.3 0.809 25.41 ± 0.07 16.16 ± 0.66 2.43 ± 0.42 25.62 11.3 2.67
dw1340+45 18.28 18.14 11.5 0.136 23.48 ± 0.06 5.76 ± 0.29 1.25 ± 0.18 24.24 6.61 2.44
M 63 subgroup
dw1255+40 18.41 17.82 11.9 0.594 25.88 ± 0.14 25.14 ± 2.48 1.34 ± 0.42 26.49 21.6 2.97
dw1303+42 18.06 17.29 12.5 0.770 24.13 ± 0.06 12.19 ± 0.54 1.61 ± 0.12 24.56 11.3 2.69
dw1305+38 17.69 17.51 12.3 0.178 21.57 ± 1.37 1.31 ± 1.87 0.59 ± 0.23 24.41 9.57 2.62
dw1305+41 17.06 16.70 13.1 0.354 23.12 ± 0.06 8.21 ± 0.53 0.94 ± 0.05 24.14 12.2 2.72
dw1308+40 18.19 17.54 12.2 0.650 23.84 ± 0.07 8.81 ± 0.60 1.11 ± 0.07 24.74 11.0 2.68

Notes. The quantities listed are as follows: (1) name of candidate; (2+3) total apparent magnitude in the g and r bands; (4) absolute r band magnitude. For candidates of the M 101 subgroup, the mean distance of the M 101 group (6.95 Mpc) is assumed; for candidates of the M 51 and M 63 subgroups, the distances of these major galaxies is 8.6 and 9.0 Mpc, respectively; (5) integrated gr color; (6) Sérsic central surface brightness in the r band; (7) Sérsic scale length in the r band; (8) Sérsic curvature index in the r band; (9) mean effective surface brightness in the r band; (10) effective radius in the r band. These photometric data are used in the Sect. 6.1 to assess the M 101 group complex membership of the candidates; (11) the logarithm of the effective radius in the r band, converted to pc with a distance assumption according to the subgroup.

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