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Table 2.

5σconf classical confusion limits (Sect. 3.3) obtained with our minimal source extractor in intensity (I) and polarization (P), together with the 50% and 80% completeness flux densities (Sect. 3.5) and the source surface density.

Band Type Central 5-σ 50% 80% Surface
name wavelength limit comp. comp. density
μm mJy mJy mJy deg−2
PHI1_1 I 25.0 0.021 0.02 0.046 43 962
PHI1_2 I 27.8 0.027 0.027 0.055 39 602
PHI1_3 I 30.9 0.037 0.037 0.07 35 070
PHI1_4 I 34.3 0.051 0.051 0.091 30 680
PHI1_5 I 38.1 0.072 0.071 0.11 26 357
PHI1_6 I 42.6 0.11 0.1 0.16 22 080
PHI2_1 I 47.4 0.16 0.16 0.25 18 089
PHI2_2 I 52.3 0.25 0.25 0.35 15 281
PHI2_3 I 58.1 0.4 0.39 0.54 12 722
PHI2_4 I 64.5 0.66 0.64 0.82 10 498
PHI2_5 I 71.7 1.1 1.1 1.4 8545
PHI2_6 I 79.7 1.9 1.8 2.1 6890

PPI1 I 96.3 4.6 4.4 5.1 4346
PPI2 I 126.0 12 11 13 2227
PPI3 I 172.0 28 27 30 908
PPI4 I 235.0 46 42 49 306

PPI1 P 96.3 0.03 0.032 0.041 5898
PPI2 P 126.0 0.078 0.082 0.096 3326
PPI3 P 172.0 0.17 0.18 0.21 1582
PPI4 P 235.0 0.25 0.27 0.32 697

Notes. The polarized flux density is assumed to be in average 1% of the photometric flux density of a galaxy.

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