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Table A.2

Flux densities used in this work for the IFRS located in the CDFS.

IFRS S 150 MHz S 200 MHz S 325 MHz S 610 MHz S 843 MHz S 844 MHz S 1.4 GHz S 2.3 GHz
ID [mJy] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy]
CS94 89 ± 27 < 104⋆ af ... < 55.6 < 27.7⋆ 11.96 ± 0.57 8.12 ± 0.93
CS97 27 ± 9 < 16 16.4 ± 4.1 6.1 ± 1.4 < 8.6 5.9 ± 1.0 4.45 ± 0.23 2.11 ± 0.26
CS114 < 29 < 17 31.1 ± 7.8 16.1 ± 3.7 14.8 ± 3.6 11.1 ± 1.4 7.34 ± 0.38 3.02 ± 0.36
CS164 < 8 < 16 0.8 ± 0.4 1.8 ± 0.6 < 6.4 1.7 ± 0.8 1.29 ± 0.07 0.81 ± 0.16
CS194 63 ± 28 < 27 23.8 ± 6.0 11.5 ± 2.9 < 14.1 7.4 ± 1.7 5.98 ± 0.31 3.10 ± 0.37
CS215 < 195⋆ < 146⋆ < 102.4⋆ ... < 32.6⋆ < 51.0⋆ 2.03 ± 0.11 < 13.29⋆
CS241 < 13 < 24 8.1 ± 2.1 1.2 ± 0.3 < 7.3 < 1.8 1.08 ± 0.06 0.43 ± 0.14
CS265 161 ± 41 104 ± 10 91.0 ± 22.7 27.8 ± 7.0 29.9 ± 3.8 29.7 ± 3.2 18.80 ± 0.82 12.10 ± 1.22
CS292 252 ± 63 159 ± 8 104.2 ± 26.1 60.7 ± 15.2 38.9 ± 4.3 37.3 ± 3.9 21.99 ± 0.80 12.22 ± 1.27
CS415 < 7 < 17 8.3 ± 2.1 ... < 5.5 < 7.1⋆ 1.38 ± 0.08 0.90 ± 0.22
CS520 37 ± 10 < 17 18.8 ± 4.7 ... 7.0 ± 4.1 5.0 ± 0.9 4.19 ± 0.22 2.17 ± 0.27
CS538 < 9 < 16 8.2 ± 2.1 ... < 5.4 < 3.9⋆ 1.14 ± 0.06 < 1.06⋆
CS539 82 ± 21 57 ± 6 45.0 ± 11.3 ... 18.3 ± 4.3 14.2 ± 1.6 9.82 ± 0.50 4.72 ± 0.53
CS574 55 ± 12 46 ± 7 49.4 ± 12.3 ... 22.9 ± 3.9 19.1 ± 2.0 12.35 ± 0.63 8.24 ± 0.84
CS603 78 ± 20 58 ± 6 52.5 ± 13.1 ... 28.5 ± 5.0 18.6 ± 2.0 11.90 ± 0.61 9.55 ± 0.97
CS618 441 ± 111 298 ± 10 236.3 ± 59.1 69.2 ± 17.3 85.8 ± 9.2 84.8 ± 8.6 47.47 ± 1.68 25.90 ± 2.65
CS649 < 7 < 17 16.8 ± 4.2 ... < 6.5 8.5 ± 1.2 6.26 ± 0.32 3.88 ± 0.43
CS703 232 ± 58 149 ± 7 128.5 ± 32.1 43.5 ± 10.9 ... 42.1 ± 4.3 22.93 ± 1.18 15.18 ± 1.56
CS713 69 ± 18 45 ± 7 54.4 ± 13.6 30.0 ± 7.5 ... 22.6 ± 2.4 16.62 ± 0.85 11.42 ± 1.18
IFRS S 4.8 GHz S 5.5 GHz S 8.6 GHz S 9 GHz S 18 GHz S 20 GHz S 34 GHz
ID [mJy] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy]
CS94 ... ... ... ... ... ... ... −0.79 ± 0.17
CS97 ... ... ... ... ... < 2.0 ... −0.91 ± 0.10
CS114 2.07 ± 0.36 ... 0.50 ± 0.19 ... ... < 2.0 0.120 ± 0.036 a −1.33 ± 0.02
CS164 0.76 ± 0.19 ... 0.21 ± 0.11 ... ... < 2.0 ... −0.26 ± 0.13
CS194 1.69 ± 0.23 ... 1.19 ± 0.25 ... ... < 2.0 0.205 ± 0.034 −1.01 ± 0.05
CS215 0.73 ± 0.17 ... 0.28 ± 0.15 ... ... ... ... −0.71 ± 0.04
CS241 < 0.24 ... < 0.21 ... ... < 2.0 ... −1.05 ± 0.19
CS265 ... 6.33 ± 0.34 ... 3.83 ± 0.25 2.18 ± 0.16 2.42 ± 0.34 ... −0.71 ± 0.01
CS292 ... ... ... ... ... ... ... −0.79 ± 0.02
CS415 < 0.33 0.429 ± 0.020 < 0.27 ... ... < 2.0 ... −1.19 ± 0.56
CS520 ... 1.292 ± 0.013 ... ... ... < 2.0 ... −1.02 ± 0.08
CS538 < 0.21 ... < 0.27 ... ... < 2.0 ... −1.19 ± 0.08
CS539 ... ... ... ... ... ... ... −0.89 ± 0.04
CS574 ... ... ... ... ... < 2.0 ... −0.81 ± 0.01
CS603 ... 6.90 ± 0.39 ... 5.00 ± 0.32 4.30 ± 0.29 5.25 ± 0.48 ... −0.65 ± 0.01
CS618 ... ... ... ... ... ... ... ...
CS649 ... ... ... ... ... < 2.0 ... −0.42 ± 0.03
CS703 8.60 ± 0.82 ... 4.22 ± 0.37 ... ... ... 1.150 ± 0.118 −0.97 ± 0.01
CS713 ... ... ... ... ... ... ... −0.61 ± 0.03

Notes. S200 MHz denotes the GLEAM flux density in the deep image (60 MHz bandwidth). The last column lists the ATLAS DR3 in-band spectral index between 1.40 GHz and 1.71 GHz. Flux density upper limits resulting from confusion are marked by (⋆). Sources for which the flux density could not be measured at the respective frequency because of image artefacts are marked by “af”. Sources that were outside the survey fields or not targeted by the observations at the respective frequency are represented by ellipsis dots (...).

(a)

Detection at 33 GHz.

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