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Table A.1

Properties of the fLSBs with photo-z < 0.2 (objects #1 to #55).

Nb RA (J2000.0) Dec (J2000.0) u err(u) g err(g′) r err(r′) i err(i′) Photo-z

1 67.9070  −13.0796 23.91 0.04 22.75 0.02 22.37 0.02 22.02 0.01 0.09
2 67.9083  −12.7808 23.26 0.03 22.59 0.02 22.50 0.02 22.62 88.00 0.19
3 67.9100  −12.8342 23.26 0.03 22.26 0.02 22.08 0.01 22.56 88.00 0.13
4 67.9101  −13.0875 24.23 0.04 23.21 0.03 22.69 0.02 22.52 0.02 0.12
5 67.9145  −13.5382 23.60 0.04 22.79 0.03 22.45 0.02 22.51 88.00 0.02
6 67.9160  −13.1696 26.29 0.25 25.34 0.11 25.32 0.13 27.15 88.00 0.16
7 67.9191  −13.7203 23.09 0.04 22.10 0.02 21.78 0.02 21.71 0.01 0.15
8 67.9262  −12.7923 24.34 0.05 23.34 0.03 23.14 0.03 23.04 88.00 0.11
9 67.9270  −13.2932 23.86 0.04 23.63 0.04 24.15 0.16 24.21 0.23 0.11
10 67.9505  −13.1668 24.04 0.04 23.15 0.03 22.69 0.02 22.72 0.02 0.16
11 67.9619  −13.7119 25.21 0.18 24.83 0.14 24.13 0.09 25.27 0.15 0.10
12 67.9875  −13.2860 24.42 0.06 23.32 0.03 22.77 0.02 22.61 0.02 0.10
13 67.9895  −12.9471 23.48 0.03 22.16 0.02 21.73 0.01 20.87 88.00 0.11
14 67.9902  −13.2069 24.75 0.07 23.76 0.04 23.40 0.03 22.83 0.02 0.11
15 68.0028  −12.9718 24.47 0.06 23.44 0.03 23.06 0.03 23.16 0.03 0.14
16 68.0050  −13.1984 24.09 0.05 22.93 0.02 22.66 0.03 23.93 0.27 0.16
17 68.0236  −12.7699 24.40 0.05 23.05 0.02 22.54 0.02 22.48 88.00 0.12
18 68.0237  −12.9592 24.63 0.06 23.54 0.03 23.38 0.03 23.02 0.02 0.11
19 68.0283  −12.8521 24.21 0.06 23.08 0.02 22.60 0.02 23.02 88.00 0.14
20 68.0370  −12.7976 23.70 0.04 22.77 0.02 22.53 0.02 22.46 88.00 0.16
21 68.0406  −12.9270 24.07 0.04 22.86 0.02 22.31 0.02 21.76 88.00 0.09
22 68.0476  −12.8429 25.75 0.16 25.62 0.12 25.61 0.18 25.10 88.00 0.09
23 68.0510  −13.6045 22.37 0.02 21.76 0.02 21.57 0.01 21.55 0.01 0.14
24 68.0940  −12.9525 25.07 0.15 24.42 0.07 24.68 0.14 23.78 0.09 0.07
25 68.0952  −12.8815 22.99 0.03 22.01 0.01 21.71 0.01 20.95 88.00 0.16
26 68.0961  −12.8760 24.68 0.06 23.73 0.03 23.11 0.02 23.35 88.00 0.12
27 68.1047  −13.0568 24.65 0.08 23.23 0.03 22.82 0.02 22.21 0.01 0.09
28 68.1090  −13.3357 24.52 0.07 23.03 0.03 22.58 0.02 22.25 0.02 0.11
29 68.1514  −12.9756 24.39 0.05 23.24 0.02 22.64 0.02 22.43 0.02 0.14
30 68.1568  −13.1103 24.04 0.05 23.11 0.03 22.63 0.02 21.79 88.00 0.17
31 68.1588  −13.3780 23.63 0.11 22.98 0.06 22.89 0.06 22.60 0.04 0.15
32 68.1594  −13.3791 24.55 0.08 23.41 0.04 23.02 0.03 23.08 88.00 0.15
33 68.1613  −13.3818 23.93 0.06 22.64 0.02 22.19 0.02 21.86 0.01 0.02
34 68.1754  −13.4260 23.61 0.04 22.76 0.02 22.35 0.02 21.90 88.00 0.12
35 68.2036  −13.0714 24.18 0.05 23.11 0.03 22.65 0.02 22.46 0.02 0.16
36 68.2042  −13.3027 24.57 0.08 23.37 0.03 22.82 0.02 22.78 88.00 0.10
37 68.2249  −12.8091 23.78 0.04 22.93 0.02 22.47 0.02 21.74 88.00 0.07
38 68.2366  −12.8454 24.16 0.06 22.77 0.02 22.26 0.02 21.26 88.00 0.13
39 68.2472  −13.1603 24.33 0.04 24.39 0.05 24.03 0.05 23.16 0.02 0.18
40 68.2507  −13.2009 23.55 0.03 23.25 0.03 22.79 0.02 22.54 0.02 0.11
41 68.2641  −13.3386 25.03 0.14 23.36 0.04 22.90 0.04 22.54 0.02 0.11
42 68.2670  −13.1963 24.47 0.07 23.11 0.02 22.49 0.02 22.27 0.02 0.18
43 68.2774  −13.3377 23.41 0.06 22.68 0.04 22.41 0.04 22.28 0.05 0.05
44 68.2802  −13.1144 24.54 0.06 24.90 0.10 24.12 0.06 23.81 0.07 0.10
45 68.2808  −13.3331 24.58 0.09 23.22 0.04 22.70 0.04 22.42 0.05 0.12
46 68.2887  −13.3069 23.12 0.09 22.68 0.04 22.26 0.05 21.91 0.03 0.01
47 68.2919  −13.5850 23.96 0.07 23.23 0.06 22.68 0.05 22.57 0.03 0.16
48 68.2966  −12.8462 23.90 0.04 22.89 0.02 22.52 0.02 22.29 0.02 0.15
49 68.2972  −13.1187 24.68 0.09 23.23 0.03 22.76 0.02 22.52 0.02 0.09
50 68.3089  −13.3587 24.74 0.07 23.47 0.03 22.92 0.02 22.64 0.02 0.11
51 68.3124  −12.8893 24.48 0.05 23.65 0.03 23.37 0.03 23.16 88.00 0.16
52 68.3162  −12.9501 27.03 0.31 26.43 0.20 25.93 0.13 25.37 0.09 0.07
53 68.3219  −13.0564 23.55 0.03 22.59 0.02 22.02 0.01 21.77 0.01 0.12
54 68.3289  −13.4163 24.22 0.08 23.28 0.04 23.21 0.04 23.01 0.03 0.13
55 68.3331  −13.4824 24.94 0.16 25.19 0.16 24.75 0.13 24.57 0.10 0.01

Notes. The columns are: (1) running number; (2) and (3) right ascension and declination for equinox J2000.0; (4) to (11) magnitudes in the four bands and corresponding errors; (12) photometric redshift. Magnitude errors of 88.00 correspond to the fLSBs for which the brightness profile fit by a Gaussian did not converge (see Sect. 2.3).

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