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Home All issues Volume 615 (July 2018) A&A, 615 (2018) A105 Full HTML
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Table A.2

Photometric and structural parameters of the new dwarf candidates in the surveyed region of the Leo-I group.

Name gtot rtot Ag Ar Mr μ0,r r0,r nr reff,r logreff,r
mag mag 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) (12) (13)
M 96 subgroup
dw1037+09 17.61 17.09 0.080 0.056 –13.04 0.496 24.04 ± 0.05 9.96 ± 0.38 1.68 ± 0.14 25.44 18.7 2.97
dw1044+11 19.39 19.17 0.088 0.061 –10.97 0.200 25.42 ± 0.45 10.87 ± 5.89 0.87 ± 0.40 26.59 12.1 2.78
dw1045+14a 19.02 18.68 0.097 0.067 –11.46 0.313 22.79 ± 0.63 1.25 ± 1.14 0.56 ± 0.16 24.87 6.92 2.54
dw1045+14b 19.79 19.29 0.094 0.065 –10.85 0.470 24.50 ± 0.17 5.24 ± 0.83 1.13 ± 0.18 25.39 6.61 2.52
dw1045+16 18.50 17.62 0.085 0.059 –12.51 0.854 24.59 ± 0.30 8.39 ± 3.22 0.81 ± 0.24 26.43 23.0 3.06
dw1045+13 18.81 18.08 0.110 0.076 –12.07 0.696 24.96 ± 0.15 7.41 ± 0.70 1.92 ± 0.52 26.59 20.0 3.00
dw1047+16 18.07 17.91 0.091 0.063 –12.23 0.128 22.77 ± 0.55 1.32 ± 1.18 0.49 ± 0.13 25.17 11.2 2.75
dw1048+13 19.83 18.67 0.111 0.077 –11.48 1.126 25.53 ± 0.10 13.63 ± 0.64 2.94 ± 0.78 26.19 12.6 2.80
dw1049+12a 19.39 18.98 0.088 0.061 –11.16 0.386 23.78 ± 0.49 2.92 ± 1.91 0.67 ± 0.19 25.54 8.18 2.61
dw1049+15 18.56 17.88 0.088 0.061 –12.26 0.655 24.30 ± 0.12 9.38 ± 0.90 1.42 ± 0.23 25.08 10.9 2.74
dw1049+12b 19.10 18.05 0.085 0.059 –12.08 1.020 24.74 ± 0.28 9.76 ± 3.03 0.96 ± 0.36 26.04 15.7 2.90
dw1051+11 17.85 16.95 0.092 0.063 –13.19 0.872 25.34 ± 0.07 16.76 ± 0.63 4.15 ± 1.20 26.20 28.2 3.15
dw1055+11 17.59 16.40 0.066 0.046 –13.72 1.169 24.88 ± 0.28 18.86 ± 3.90 0.97 ± 0.54 26.18 36.0 3.25
dw1059+11 18.98 18.60 0.060 0.041 –11.51 0.359 24.61 ± 0.11 9.73 ± 0.72 1.68 ± 0.26 25.02 7.65 2.58
dw1101+11 19.47 19.45 0.058 0.040 –10.66 0.005 23.33 ± 1.62 1.16 ± 2.78 0.50 ± 0.32 25.56 6.64 2.52
Leo Triplet
dw1116+14 20.33 19.57 0.071 0.049 –10.56 0.742 25.67 ± 0.13 10.63 ± 0.58 3.28 ± 1.11 25.81 7.08 2.55
dw1116+15a 20.26 19.80 0.076 0.052 –10.33 0.437 25.11 ± 0.32 6.79 ± 2.43 0.95 ± 0.28 25.98 6.88 2.54
dw1116+15b 20.42 19.31 0.068 0.047 –10.81 1.091 25.33 ± 0.26 8.85 ± 2.61 1.00 ± 0.32 27.02 13.8 2.84
dw1117+15 17.56 17.25 0.082 0.057 –12.88 0.280 25.57 ± 0.07 17.11 ± 0.51 3.79 ± 0.92 27.31 40.9 3.31
dw1117+12 21.22 19.87 0.073 0.050 –10.25 1.322 25.24 ± 0.52 7.29 ± 4.29 0.93 ± 0.51 26.10 7.02 2.54
dw1118+13a 19.49 19.59 0.077 0.053 –10.54 –0.11 25.88 ± 0.24 14.36 ± 1.94 1.74 ± 1.02 26.36 9.04 2.65
dw1118+13b 18.15 17.78 0.069 0.047 –12.34 0.341 25.33 ± 0.13 15.09 ± 1.66 1.35 ± 0.24 26.45 21.5 3.03
dw1123+13 19.62 19.08 0.079 0.054 –11.05 0.513 24.95 ± 0.16 8.74 ± 1.05 1.55 ± 0.31 25.38 7.26 2.56
dw1127+13 19.76 18.85 0.093 0.064 –11.28 0.872 25.51 ± 0.13 12.85 ± 0.95 1.72 ± 0.52 26.10 11.2 2.75
Field
dw1013+18 18.02 17.65 0.106 0.073 –12.50 0.340 22.67 ± 0.10 3.29 ± 0.38 0.76 ± 0.04 24.16 7.99 2.60
dw1040+06 17.96 18.22 0.120 0.083 –11.94 –0.29 24.36 ± 0.12 8.18 ± 0.88 1.20 ± 0.17 25.37 10.7 2.73
dw1109+18 17.73 17.18 0.077 0.054 –12.95 0.523 23.25 ± 0.06 7.35 ± 0.41 1.07 ± 0.06 24.17 9.94 2.70
dw1110+18 18.00 17.39 0.077 0.053 –12.74 0.587 24.30 ± 0.11 12.15 ± 1.16 1.20 ± 0.20 25.15 14.2 2.85
dw1130+20 17.53 17.28 0.068 0.047 –12.84 0.220 22.63 ± 0.14 2.75 ± 0.58 0.61 ± 0.05 24.49 10.9 2.74
dw1131+15 19.51 18.87 0.171 0.118 –11.32 0.581 24.59 ± 0.09 7.39 ± 0.42 1.97 ± 0.24 25.22 7.43 2.57
dw1137+16 17.32 16.77 0.097 0.067 –13.37 0.523 24.49 ± 0.12 14.19 ± 1.99 0.89 ± 0.10 25.89 26.6 3.12
dw1140+17 18.54 17.89 0.098 0.068 –12.25 0.623 24.85 ± 0.20 13.96 ± 3.30 0.87 ± 0.23 25.67 14.3 2.85
dw1145+14 19.86 19.20 0.147 0.101 –10.97 0.613 24.02 ± 0.12 4.94 ± 0.49 1.39 ± 0.17 24.65 4.89 2.39
dw1148+12 17.95 17.91 0.119 0.082 –12.25 0.002 24.58 ± 0.20 9.02 ± 1.75 1.02 ± 0.29 25.78 14.9 2.87
dw1148+16 17.49 17.34 0.150 0.104 –12.84 0.109 22.85 ± 0.06 3.77 ± 0.32 0.78 ± 0.04 24.61 11.3 2.75
dw1151+16 18.04 18.27 0.109 0.075 –11.88 –0.25 22.92 ± 0.07 3.92 ± 0.25 1.09 ± 0.05 23.86 5.24 2.42

Notes.The quantities listed are as follows: (1) name of candidate; (2–3) total apparent magnitude in the g and r bands; (4–5) galactic extinction in the g and r bands (Schlafly & Finkbeiner 2011); (6) extinction corrected absolute r band magnitude, using a distance modulus of M − m = 30.06 mag; (7) integrated and extinction corrected g − r color; (8) Sérsic central surface brightness in the r band; (9) Sérsic scale length in the r band; (10) Sérsic curvature index in the r band; (11) mean effective surface brightness in the r band; (12) effective radius in the r band; (13) the logarithm of the effective radius in the r band, converted to pc with a distance modulus of M − m = 30.06 mag. We note that surface brightness values presented are not extinction corrected.

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