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Table A.5.
Parameters related to the star formation estimation for our sample.
| Short name | W3 | W4 | W3-W4 | SW3 | S20cm CDFS | S20 cm ELAIS | q22 |
|---|---|---|---|---|---|---|---|
| (mag) | (mag) | (mag) | (mJy) | (mJy) | (mJy) | ||
| J0347+0105 | 5.32 ± 0.02 | 3.03 ± 0.02 | 2.29 ± 0.05 | 234.80 ± 3.46 | 21.03 ± 1.43 | 20.01 ± 2.44 | 1.21 |
| J0629-0545 | 5.48 ± 0.02 | 2.60 ± 0.02 | 2.88 ± 0.08 | 203.38 ± 2.44 | 31.36 ± 2.11 | 29.82 ± 3.61 | 1.19 |
| J0632+6340 | 6.28 ± 0.02 | 3.76 ± 0.02 | 2.52 ± 0.06 | 97.43 ± 1.35 | 10.74 ± 0.71 | 10.23 ± 1.23 | 1.65 |
| J0706+3901 | 8.60 ± 0.03 | 6.05 ± 0.05 | 2.55 ± 0.14 | 11.51 ± 0.28 | 1.31 ± 0.13 | 1.25 ± 0.19 | 0.70 |
| J0713+3820 | 6.26 ± 0.02 | 3.98 ± 0.02 | 2.28 ± 0.05 | 99.15 ± 1.37 | 8.74 ± 0.60 | 8.32 ± 1.02 | 1.19 |
| J0804+3853 | 8.08 ± 0.02 | 5.37 ± 0.03 | 2.70 ± 0.10 | 18.62 ± 0.38 | 2.44 ± 0.19 | 2.32 ± 0.31 | 1.36 |
| J0806+7248 | 8.11 ± 0.02 | 5.54 ± 0.04 | 2.57 ± 0.11 | 17.99 ± 0.40 | 2.08 ± 0.18 | 1.99 ± 0.28 | 0.11 |
| J0814+5609 | 10.41 ± 0.07 | 8.43 ± 0.45 | 1.98 ± 0.66 | 2.17 ± 0.15 | 0.15 ± 0.07 | 0.15 ± 0.08 | -0.99 |
| J0913+3658 | 8.20 ± 0.02 | 5.65 ± 0.04 | 2.55 ± 0.11 | 16.67 ± 0.32 | 1.89 ± 0.16 | 1.80 ± 0.25 | 1.67 |
| J0925+5217 | 6.72 ± 0.02 | 4.71 ± 0.03 | 2.01 ± 0.05 | 64.67 ± 1.01 | 4.46 ± 0.34 | 4.25 ± 0.56 | 1.35 |
| J0926+1244 | 6.16 ± 0.02 | 3.80 ± 0.02 | 2.36 ± 0.05 | 108.92 ± 1.50 | 10.40 ± 0.75 | 9.90 ± 1.25 | 1.54 |
| J0937+3615 | 8.14 ± 0.02 | 5.47 ± 0.04 | 2.66 ± 0.12 | 17.65 ± 0.34 | 2.22 ± 0.18 | 2.12 ± 0.29 | 1.34 |
| J0952-0136 | 4.33 ± 0.01 | 2.31 ± 0.02 | 2.02 ± 0.04 | 589.25 ± 7.60 | 40.81 ± 2.56 | 38.83 ± 4.52 | 1.16 |
| J1034+3938 | 6.65 ± 0.02 | 4.51 ± 0.03 | 2.14 ± 0.06 | 69.49 ± 0.96 | 5.40 ± 0.40 | 5.14 ± 0.66 | 0.57 |
| J1038+4227 | 8.87 ± 0.03 | 6.58 ± 0.06 | 2.29 ± 0.13 | 8.97 ± 0.23 | 0.80 ± 0.08 | 0.77 ± 0.12 | 0.07 |
| J1047+4725 | 10.44 ± 0.09 | 7.75 ± 0.19 | 2.69 ± 0.52 | 2.12 ± 0.17 | 0.27 ± 0.06 | 0.27 ± 0.08 | -2.18 |
| J1048+2222 | 9.29 ± 0.04 | 7.08 ± 0.11 | 2.20 ± 0.21 | 6.08 ± 0.25 | 0.50 ± 0.08 | 0.48 ± 0.10 | 1.09 |
| J1102+2239 | 9.15 ± 0.03 | 6.49 ± 0.07 | 2.66 ± 0.20 | 6.96 ± 0.22 | 0.87 ± 0.10 | 0.83 ± 0.14 | 0.81 |
| J1110+3653 | nd | nd | N/A | N/A | N/A | N/A | N/A |
| J1121+5351 | 7.32 ± 0.02 | 4.99 ± 0.03 | 2.33 ± 0.07 | 37.39 ± 0.62 | 3.46 ± 0.27 | 3.30 ± 0.44 | 1.48 |
| J1138+3653 | 10.53 ± 0.08 | 8.01 ± 0.21 | 2.52 ± 0.50 | 1.94 ± 0.15 | 0.22 ± 0.05 | 0.21 ± 0.06 | -0.28 |
| J1159+2838 | 9.02 ± 0.03 | 5.98 ± 0.04 | 3.03 ± 0.17 | 7.85 ± 0.25 | 1.39 ± 0.12 | 1.33 ± 0.19 | 1.22 |
| J1203+4431 | 4.58 ± 0.02 | 2.16 ± 0.02 | 2.41 ± 0.05 | 468.06 ± 6.47 | 46.81 ± 2.97 | 44.53 ± 5.23 | 1.96 |
| J1209+3217 | 8.18 ± 0.02 | 5.30 ± 0.03 | 2.88 ± 0.11 | 16.93 ± 0.33 | 2.60 ± 0.20 | 2.48 ± 0.32 | 1.75 |
| J1215+5442 | 7.48 ± 0.02 | 5.01 ± 0.04 | 2.47 ± 0.10 | 32.17 ± 0.53 | 3.40 ± 0.28 | 3.24 ± 0.44 | 1.52 |
| J1218+2948 | 5.00 ± 0.01 | 2.13 ± 0.02 | 2.87 ± 0.07 | 316.16 ± 4.08 | 48.08 ± 3.23 | 45.74 ± 5.54 | 1.40 |
| J1227+3214 | 7.42 ± 0.02 | 4.80 ± 0.02 | 2.62 ± 0.06 | 34.10 ± 0.57 | 4.12 ± 0.29 | 3.92 ± 0.49 | 1.06 |
| J1242+3317 | 6.70 ± 0.02 | 3.98 ± 0.02 | 2.72 ± 0.07 | 66.30 ± 0.98 | 8.82 ± 0.62 | 8.39 ± 1.04 | 1.59 |
| J1246+0222 | 7.22 ± 0.02 | 4.66 ± 0.03 | 2.56 ± 0.08 | 40.95 ± 0.64 | 4.69 ± 0.34 | 4.46 ± 0.57 | 2.26 |
| J1302+1624 | 7.88 ± 0.02 | 5.26 ± 0.04 | 2.62 ± 0.12 | 22.28 ± 0.41 | 2.70 ± 0.22 | 2.58 ± 0.35 | -0.11 |
| J1305+5116 | 8.91 ± 0.03 | 6.57 ± 0.07 | 2.34 ± 0.16 | 8.63 ± 0.21 | 0.81 ± 0.09 | 0.78 ± 0.13 | -0.61 |
| J1317+6010 | 8.40 ± 0.02 | 5.80 ± 0.04 | 2.60 ± 0.11 | 13.79 ± 0.27 | 1.64 ± 0.14 | 1.57 ± 0.22 | 1.60 |
| J1337+2423 | 4.59 ± 0.01 | 2.66 ± 0.02 | 1.95 ± 0.03 | 462.06 ± 5.96 | 30.03 ± 1.91 | 28.57 ± 3.35 | 1.29 |
| J1348+2622 | 10.40 ± 0.06 | 8.57 ± 0.29 | 1.83 ± 0.40 | 2.19 ± 0.13 | 0.13 ± 0.04 | 0.13 ± 0.05 | 0.32 |
| J1358+2658 | 9.22 ± 0.03 | 6.53 ± 0.06 | 2.69 ± 0.18 | 6.47 ± 0.18 | 0.84 ± 0.09 | 0.80 ± 0.13 | 1.30 |
| J1402+2159 | 7.18 ± 0.02 | 4.34 ± 0.03 | 2.75 ± 0.11 | 42.41 ± 0.63 | 5.78 ± 0.43 | 5.50 ± 0.70 | 2.16 |
| J1536+5433 | 6.95 ± 0.02 | 5.02 ± 0.02 | 1.92 ± 0.04 | 52.76 ± 0.78 | 3.36 ± 0.23 | 3.20 ± 0.40 | 2.12 |
| J1555+1911 | 7.97 ± 0.02 | 5.35 ± 0.04 | 2.62 ± 0.12 | 20.47 ± 0.38 | 2.49 ± 0.20 | 2.37 ± 0.32 | 1.67 |
| J1559+3501 | 6.62 ± 0.02 | 4.28 ± 0.02 | 2.34 ± 0.05 | 71.04 ± 0.98 | 6.64 ± 0.47 | 6.33 ± 0.78 | 1.38 |
| J1633+4718 | 7.64 ± 0.02 | 4.97 ± 0.02 | 2.67 ± 0.06 | 27.79 ± 0.44 | 3.51 ± 0.25 | 3.35 ± 0.42 | 0.22 |
| J1703+4540 | 6.01 ± 0.02 | 3.42 ± 0.02 | 2.59 ± 0.06 | 125.17 ± 1.73 | 14.75 ± 0.98 | 14.04 ± 1.69 | 0.52 |
| J1713+3523 | 7.48 ± 0.02 | 5.38 ± 0.03 | 2.11 ± 0.06 | 32.11 ± 0.53 | 2.43 ± 0.20 | 2.32 ± 0.31 | 0.62 |
| J2242+2943 | 5.78 ± 0.01 | 3.21 ± 0.02 | 2.57 ± 0.06 | 153.99 ± 1.84 | 17.80 ± 1.16 | 16.94 ± 2.02 | 1.16 |
| J2314+2243 | 6.74 ± 0.02 | 4.40 ± 0.03 | 2.33 ± 0.07 | 64.08 ± 0.94 | 5.93 ± 0.43 | 5.65 ± 0.72 | 0.85 |
Notes. (1) Short name, (2) WISE W3-band magnitude, (3) WISE W4-band magnitude, (4) WISE W3-W4 magnitude colour, (5) WISE W3-band flux density in mJy (6) 20 cm flux density in mJy estimated from the WISE W4-band flux density, using a relation based on CDFS data (Boyle et al. 2007), (7) 20 cm flux density in mJy estimated from the WISE W4-band flux density, using a relation based on ELAIS data (Boyle et al. 2007), (8) q22 parameter = log (S22μm /S1.4 GHz).
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