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Table A.1

Flux densities used in this work for the IFRS located in the ELAIS-S1 field.

IFRS S200 MHz S610 MHz S843 MHz S1.4 GHz S2.3 GHz S4.8 GHz S8.6 GHz S34 GHz
ID [mJy] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy] [mJy]

ES5 143 ± 8 26.6 ± 6.7 22.5 ± 2.0 11.51 ± 0.49 5.21 ± 0.72 ... ... ... ...
ES66 147 ± 9 67.0 ± 19.6 61.6 ± 4.5 34.37 ± 1.74 20.84 ± 2.16 ... ... ... ...
ES201 46 ± 13 8.5 ± 2.1 < 11.3 4.62 ± 0.23 2.18 ± 0.26 ... ... ... −1.26 ± 0.12
ES419 < 21 2.2 ± 0.6 < 4.3 1.45 ± 0.09 < 1.31 < 0.39 < 0.33 ... −1.07 ± 0.45
ES427 119 ± 8 47.7 ± 11.9 36.8 ± 2.1 21.42 ± 1.10 12.63 ± 1.26 6.54 ± 0.46 2.83 ± 0.36 0.575 ± 0.098 −0.95 ± 0.10
ES509 120 ± 8 49.2 ± 12.3 36.6 ± 2.2 21.75 ± 1.11 13.18 ± 1.33 5.94 ± 0.45 3.51 ± 0.39 0.550 ± 0.096 −0.99 ± 0.10
ES645 < 20 10.7 ± 3.1 8.5 ± 2.7 4.66 ± 0.25 2.67 ± 0.41 ... ... ... 0.05 ± 0.33
ES749 60 ± 15 15.7 ± 4.7 12.6 ± 1.7 9.22 ± 0.62 4.99 ± 0.69 2.63 ± 0.29 0.82 ± 0.26 ... ...
ES798 60 ± 11 14.6 ± 3.7 12.7 ± 1.7 7.48 ± 0.38 4.37 ± 0.51 3.07 ± 0.37 < 0.33 ... −0.70 ± 0.19
ES973 < 97 12.1 ± 3.0 17.2 ± 2.6 7.83 ± 0.32 4.05 ± 0.44 1.93 ± 0.29 < 0.27 < 0.385 −0.84 ± 0.13
ES1018 113 ± 9 58.0 ± 16.9 42.0 ± 2.5 27.87 ± 1.40 18.89 ± 1.92 ... ... ... −0.74 ± 0.13
ES1021 < 131 30.3 ± 7.6 24.8 ± 1.6 15.38 ± 0.69 10.88 ± 1.09 ... ... ... −0.76 ± 0.10
ES1156 35 ± 7 55.1 ± 13.8 46.6 ± 2.9 31.22 ± 1.60 20.13 ± 2.02 ... ... ... −0.81 ± 0.10
ES1239 111 ± 8 48.9 ± 14.3 37.1 ± 2.3 21.72 ± 1.11 15.31 ± 1.54 ... ... ... −0.83 ± 0.10
ES1259 67 ± 10 ... af 4.08 ± 0.22 2.31 ± 0.82 ... ... ... ...

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 (...).

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