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Table 1.

Radio properties of our LzLCS sample.

Object Flux density at 3 GHz Flux density at 6 GHz Flux density at 1.5 GHz α 6 GHz 3 GHz $ \alpha^{\mathrm{3\,GHz}}_{\mathrm{6\,GHz}} $
(μJy) (μJy) (μJy)
J004743+015440 < 28.5 24.0 ± 5.5 < 90.0 ≤0.25
J011309+000223 < 31.2 (a) < 63.0
J012910+145935 < 45.0 75.6 ± 7.0 < 63.0 < 0.75
J072326+414608 87.2 ± 8.1 < 16.5 < 42.0 ≥2.4
J081112+414146 < 44.4 < 19.5 < 42.0
J081409+211459 142.0 ± 8.8 114.3 ± 5.2 300.0 ± 8.0 −0.313 ± 0.033
J082652+182052 69.4 ± 8.9 37.0 ± 6.6 < 27.0 −0.907 ± 0.209
J083440+480541 68.2 ± 7.8 69.1 ± 5.1 143.0 ± 15.0 0.019 ± 0.003
J090918+392925 < 25.5 < 17.4 < 45.0
J091113+183108 69.2 ± 8.5 52.7 ± 5.0 < 90.0 (b) −0.393 ± 0.067
J091207+523960 (a) < 123.0
J091208+505009 < 26.1 40.0 ± 5.7 < 45.0 < 0.62
J091703+315221 55.6 ± 8.2 47.5 ± 5.8 80.0 ± 20.0 −0.227 ± 0.046
J092552+395714 < 25.8 < 16.5 < 33.0
J094001+593244 63.0 ± 10.4 26.0 ± 4.9 −1.277 ± 0.332
J095236+405249 (b) 392.3 ± 7.5 50.9 ± 5.4 < 36.0 −2.946 ± 0.38
J095700+235709 930.0 ± 81.2 210.0 ± 23.8 1730.0 ± 150.0 −2.147 ± 0.343
J095838+202508 < 25.2 < 16.5 < 30.0
J101401+523251 < 22.5 < 16.2
J102615+633308 < 25.2 < 15.6
J103344+635317 73.8 ± 8.0 80.7 ± 6.0 0.129 ± 0.019
J103816+452718 132.4 ± 8.9 40.4 ± 5.8 −1.712 ± 0.297
J105117+474357 < 27.0 < 16.8
J105331+523753 158.7 ± 8.2 79.8 ± 5.6 −0.992 ± 0.111
J110452+475204 < 23.7 < 16.2
J112224+412052 < 25.5 < 17.1
J112848+524509 < 23.1 < 16.2
J112933+493525 < 22.2 < 18.0
J113304+651341 < 24.0 27.9 ± 5.8 < 0.22
J115855+312559 136.7 ± 7.9 72.9 ± 5.6 −0.907 ± 0.108
J115959+382422 < 23.7 < 17.1
J120934+305326 120.7 ± 7.8 70.5 ± 5.5 −0.776 ± 0.096
J121915+453930 < 25.5 < 19.2
J123519+063556 < 28.5 < 19.5
J124423+021540 225.6 ± 9.2 145.7 ± 5.9 −0.631 ± 0.057
J124619+444902 61.0 ± 12.6 41.5 ± 5.0 −0.556 ± 0.139
J124835+123403 126.0 ± 7.7 76.0 ± 6.0 −0.729 ± 0.089
J124911+464535 57.0 ± 7.9 < 16.8 ≥1.76
J125718+410221 (b) 82.2 ± 9.7 26.6 ± 5.5 −1.628 ± 0.404
J130128+510451 (c) 488.0 ± 8.0 < 16.5 ≥4.89
J131037+214817 < 24.3 41.3 ± 5.6 < 0.77
J131419+104739 125.0 ± 8.3 37.7 ± 6.0 −1.729 ± 0.322
J131904+510309 98.5 ± 8.7 30.4 ± 5.0 −1.696 ± 0.339
J132633+421824 95.0 ± 8.4 < 17.1 ≥2.47
J132937+573315 132.1 ± 8.2 29.2 ± 5.6 −2.178 ± 0.465
J134559+112848 249.6 ± 7.7 71.4 ± 5.7 −1.806 ± 0.2
J141013+434435 (b) 233.0 ± 8.8 99.6 ± 5.4 −1.226 ± 0.119
J144010+461937 158.9 ± 8.3 96.7 ± 5.7 −0.717 ± 0.076
J151707+370512 < 30.0 30.7 ± 6.4 < 0.03
J155945+403325 74.8 ± 8.3 87.2 ± 5.3 0.221 ± 0.032
J160437+081959 113.6 ± 9.4 < 18.0 ≥2.66
J164607+313054 < 26.7 < 19.8
J164849+495751 < 39.9 < 38.4

Notes. For non-detections in the different bands, we present the 3σ upper limits on the flux density. For estimating the upper/lower limits on α 6 GHz 3 GHz $ \alpha^{\mathrm{3\,GHz}}_{\mathrm{6\,GHz}} $, we use the corresponding 3σ upper limits on the flux density.

(a)

Here the noise is high due to a very strong source in the field.

(b)

For these sources the flux density measurement is uncertain due to artefacts from a strong source in the field.

(c)

For this source the flux is possibly contaminated due to AGN jet from a neighbouring source. See Appendix D for more details.

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