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Table 2

Selected fields for the photometric analysis of the Galactic cirri.

Field RA (J2000) Dec (J2000) l b Area ⟨g-r⟩ ⟨r-i⟩ ⟨i-z⟩ ⟨S100μm⟩ ⟨τ353 GHz⟩
# (deg) (deg) (deg) (deg) (deg2) (mag) (mag) (mag) (MJy sr−1) (×10−6)
1 324.0 0.0 54.7 –35.8 2 0.57 ± 0.04 0.12 ± 0.04 0.00 ± 0.11 3.84 4.18
0.49 ± 0.05 0.18 ± 0.05 0.11 ± 0.19
2 333.0 –0.75 60.8 –43.6 0.75 0.60 ± 0.04 0.05 ± 0.04 0.01 ± 0.11 5.02 6.06
0.52 ± 0.04 0.13 ± 0.03 0.19 ± 0.07
3 342.75 0.25 71.4 –50.2 1.75 0.63 ± 0.04 0.13 ± 0.04 0.10 ± 0.11 5.59 7.20
0.46 ± 0.10 0.07 ± 0.10 0.12 ± 0.30
4 344.0 –0.25 72.3 –51.4 2 0.53 ± 0.04 0.12 ± 0.04 0.08 ± 0.11 4.54 5.18
0.55 ± 0.03 0.13 ± 0.02 0.11 ± 0.11
5 2.5 –0.25 100.9 –61.3 3 0.57 ± 0.04 0.06 ± 0.04 0.04 ± 0.11 3.97 2.91
0.56 ± 0.05 0.15 ± 0.04 0.02 ± 0.15
6 326.0 0.25 56.4 –37.4 2.0 0.57 ± 0.04 0.17 ± 0.04 0.11 ± 0.11 4.04 4.38
0.51 ± 0.04 0.08 ± 0.05 0.07 ± 0.09
7 327.0 0.0 56.7 –38.3 2.25 0.63 ± 0.04 0.20 ± 0.04 0.02 ± 0.11 5.82 7.38
0.66 ± 0.04 0.22 ± 0.03 0.02 ± 0.11
8 328.0 0.0 57.5 –39.0 2.5 0.67 ± 0.04 0.20 ± 0.04 0.07 ± 0.11 6.19 7.87
0.66 ± 0.03 0.30 ± 0.02 0.13 ± 0.06
9 329.0 –0.25 58.1 –40.0 1.75 0.59 ± 0.04 0.17 ± 0.04 0.10 ± 0.11 5.89 6.78
0.47 ± 0.07 0.26 ± 0.06 0.05 ± 0.24
10 330.0 –0.75 59.1 –40.7 0.75 0.57 ± 0.04 0.13 ± 0.04 0.08 ± 0.11 5.20 4.94
0.57 ± 0.10 –0.01 ± 0.20 0.25 ± 0.38
11 54.95 0.50 185.6 –41.0 1.35 0.61 ± 0.04 0.14 ± 0.04 0.09 ± 0.11 5.41 6.70
0.63 ± 0.09 0.13 ± 0.11 0.03 ± 0.15
12 55.85 0.50 186.3 –40.3 1.35 0.69 ± 0.04 0.15 ± 0.04 –0.10 ± 0.11 5.98 8.07
0.66 ± 0.08 0.16 ± 0.04 –0.01 ± 0.11
13 56.75 0.50 187.1 –39.6 1.35 0.73 ± 0.04 0.18 ± 0.04 –0.05 ± 0.11 8.28 13.63
0.60 ± 0.09 0.20 ± 0.03 –0.04 ± 0.17
14 57.65 0.50 187.8 –38.9 1.35 0.72 ± 0.04 0.17 ± 0.04 0.01 ± 0.11 9.01 16.15
0.93 ± 0.05 0.12 ± 0.09 0.12 ± 0.10
15 58.55 0.50 188.4 –38.2 1.35 0.83 ± 0.04 0.25 ± 0.04 0.05 ± 0.11 14.02 25.55
0.71 ± 0.06 0.24 ± 0.03 0.05 ± 0.11
16 59.5 –0.75 190.4 –38.1 1.0 0.92 ± 0.04 0.30 ± 0.04 0.01 ± 0.11 15.73 28.90
0.84 ± 0.09 0.23 ± 0.06 0.02 ± 0.17

Notes. Each of the optical color estimations given for each field corresponds to the value obtained by using two different methodologies: the Lorentzian + Gaussian analysis of the signal (upper values) and the flux fraction technique (bottom values). See text for details.

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