Table 2
Multi-wavelength photometric properties and photo-zs of the LOFAR-selected sample.
| Source name | S150MHz (mJy) | 4.5 μm mag | Kmag | NB921mag | i mag | z mag | photo-z | |
|---|---|---|---|---|---|---|---|---|
| z1 | z2 | |||||||
| ILTJ160227.18+544759.8 | 0.35 ± 0.04 | 19.95 ± 0.07 | 21.10 ± 0.11 | 23.18 ± 0.15 | 24.64 ± 0.43 | 23.76 ± 0.32 | 1.7 |
2.7 |
| ILTJ160658.74+550607.0 | 0.10 ± 0.04 | 20.99 ± 0.17 | 22.39 ± 0.34 | 24.48 ± 0.50 | 25.60 ± 1.04 | 25.33 ± 1.37 | 6.1 |
4.4 |
| ILTJ160930.42+544435.9 | 0.11 ± 0.05 | 20.13 ± 0.08 | 21.17 ± 0.12 | 23.19 ± 0.15 | 24.59 ± 0.41 | 23.90 ± 0.37 | 1.6 |
– |
| ILTJ161209.13+544818.7 | 0.18 ± 0.05 | 20.57 ± 0.12 | 21.65 ± 0.18 | 22.26 ± 0.06 | 23.49 ± 0.15 | 23.16 ± 0.19 | 1.4 |
0.85 |
| ILTJ161447.04+550401.8 | 0.09 ± 0.03 | 20.73 ± 0.13 | 22.16 ± 0.29 | 24.49 ± 0.50 | 25.76 ± 1.19 | 25.71 ± 1.94 | 2.1 |
4.4 |
Notes. The 4.5 μm magnitude is taken from the SWIRE survey (Lonsdale et al. 2003), and the i and z magnitudes from HSC-SSP (Aihara et al. 2018b) are both taken from the LoTSS Deep Fields catalogue (Kondapally et al. 2021). The photometric redshifts z1,median and z2,median were obtained from LoTSS Deep Fields catalogue (see D20), where z1,median and z2,median are the medians of the primary and secondary redshift peaks, respectively. A more detailed SED fitting shows that these sources are all likely [OII] emitters at z = 1.47 (see Sect. 3.1).
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