Table A.1.
Sample of candidate low-power CSOs.
| Name | mJIVE-20 name | Id. | mr | z | mW1 | Sp,1.38 | SFIRST | SVLASS |  |
LAS |
|---|---|---|---|---|---|---|---|---|---|---|
| MJV | mag | mag | mJy/b | mJy | mJy | mas | ||||
| J0802+6125 | 00141 | s | 24.37 | 1.129±0.151 | 17.52 | 5.7 | 14.6 | 7.8 | 0.8 | 28 |
| J0810+5011 | 01651 | G | 22.13 | 1.053±0.434 | 16.20 | 3.8 | 8.1 | 11.4 | −0.5 | 20 |
| J0810+4117 | 09498 | G | 23.38 | 0.957±0.158 | 16.21 | 4.9 | 13.6 | 9.3 | 0.5 | 14 |
| J0816+3616 | 04053 | E | 4.7 | 8.8 | 5.5 | 0.6 | 17 | |||
| J0834+4111 | 19180 | G | 24.28 | 1.137±0.142 | 16.22 | 39.1 | 100.6 | 56.0 | 0.7 | 22 |
| J0855+2030 | 01713 | G | 18.16 | 0.251±0.011 | 14.83 | 11.8 | 25.1 | 14.0 | 0.7 | 16 |
| J0857+2128 | 22448 | G | 21.33 | 0.857±0.055 | 16.03 | 3.2 | 12.1 | 6.2 | 0.9 | 50 |
| J0901+4256 | 17295 | Q | 19.31 | 1.011sp | 15.19 | 10.9 | 24.5 | 15.5 | 0.6 | 20 |
| J0902+4703 | 09733 | s | 23.85 | 1.020±0.155 | 14.8 | 23.6 | 19.4 | 0.3 | 25 | |
| J0917+3351 | 16793 | E | 17.30 | 8.0 | 25.8 | 14.2 | 0.8 | 34 | ||
| J0924+4035 | 14046 | G | 24.19 | 1.112±0.239 | 17.29 | 3.4 | 22.7 | 10.0 | 1.1 | 34 |
| J0941+2600 | 04207 | G | 24.09 | 1.224±0.331 | 16.97 | 2.3 | 9.9 | 4.8 | 0.9 | 20 |
| J0956+2529 | 11834 | s | 24.88 | 1.248±0.375 | 17.09 | 16.9 | 47.1 | 23.0 | 0.9 | 26 |
| J0957+2541 | 11874 | E | 99.0 | 142.5 | 96.4 | 0.5 | 26 | |||
| J0958+3208 | 04323 | G | 23.65 | 1.090±0.465 | 17.33 | 37.8 | 60.5 | 34.8 | 0.7 | 25 |
| J1008+1328 | 17434 | E | 9.1 | 17.1 | 11 | 0.6 | 22 | |||
| J1017+3532 | 08253 | G | 19.68 | 0.337sp | 15.47 | 19.0 | 28.4 | 17.0 | 0.7 | 20 |
| J1022+3459 | 15244 | Q | 19.33 | 1.935sp | 15.17 | 3.0 | 6.6 | 4.1 | 0.6 | 11 |
| J1037+0514 | 12154 | Q | 20.59 | 2.0995sp | 16.38 | 5.0 | 16.5 | 8.0 | 0.9 | 37 |
| J1041+5344 | 13694 | G | 22.40 | 1.000±0.130 | 16.36 | 4.8 | 16.4 | 9.9 | 0.6 | 26 |
| J1102+3815 | 06949 | E | 17.40 | 3.1 | 6.1 | 2.9 | 1.0 | 11 | ||
| J1107+1619 | 19609 | E | 39.1 | 96.4 | 45.0 | 1.0 | 19 | |||
| J1107+4346 | 05578 | E | 6.2 | 10.5 | 6.5 | 0.6 | 11 | |||
| J1112+1445 | 08326 | E | 2.8 | 6.4 | 4.5 | 0.5 | 30 | |||
| J1120−0607 | 10165 | E | 62.3 | 122.4 | 89.0 | 0.4 | 14 | |||
| J1127+2540 | 07057 | E | 17.23 | 19.7 | 65.5 | 31.0 | 1.0 | 55 | ||
| J1201−0503 | 12448 | G | 22.23 | 0.752±0.054 | 16.24 | 3.8 | 10.8 | 5.2 | 0.9 | 23 |
| J1206+2821 | 13722 | E | 17.6 | 56.2 | 27.0 | 1.0 | 30 | |||
| J1209+4115 | 00873 | G | 18.1 | 0.095sp | 13.18 | 68.6 | 146.8 | 120.1 | 0.3 | 25 |
| J1214+3438 | 15828 | E | 17.61 | 48.3 | 78.4 | 30.0 | 1.3 | 18 | ||
| J1217−0049 | 20203 | G | 23.38 | 0.887±0.069 | 8.0 | 13.7 | 7.3 | 0.8 | 23 | |
| J1218+3813 | 20308 | E | 6.0 | 12.1 | 7.1 | 0.7 | 20 | |||
| J1219+5845 | 12583 | E | 11.1 | 17.5 | 14.0 | 0.3 | 20 | |||
| J1230+3728 | 07332 | G | 21.89 | 0.479±0.093 | 17.26 | 42.6 | 91.0 | 46.0 | 0.9 | 21 |
| J1239+3713 | 20358 | G | 24.83 | 0.984±0.219 | 16.08 | 10.0 | 21.4 | 11.0 | 0.9 | 25 |
| J1242+3709 | 20362 | E | 4.6 | 8.4 | 5.3 | 0.6 | 9 | |||
| J1254+1156 | 07387 | G | 20.47 | 0.591±0.067 | 15.59 | 2.8 | 7.7 | 3.6 | 1.0 | 28 |
| J1257+3244 | 04612 | G | 22.38 | 0.792±0.073 | 16.67 | 2.6 | 8.1 | 5.0 | 0.6 | 37 |
| J1258+3252 | 04637 | G | 19.68 | 0.559±0.031 | 15.10 | 3.8 | 7.4 | 5.5 | 0.4 | 20 |
| J1310+1204 | 15395 | E | 7.0 | 12.8 | 6.0 | 1.0 | 25 | |||
| J1311+3221 | 02847 | G | 23.49 | 0.960±0.105 | 17.01 | 5.6 | 16.3 | 11.3 | 0.5 | 20 |
| J1334+1623 | 20701 | G | 23.91 | 16.78 | 16.0 | 26.2 | 15.2 | 0.7 | 28 | |
| J1337+4603 | 06117 | E | 17.77 | 12.7 | 27.6 | 14.4 | 0.8 | 11 | ||
| J1343+2730 | 14513 | E | 8.0 | 15.5 | 6.8 | 1.1 | 11 | |||
| J1357+1922 | 10688 | E | 7.0 | 11.5 | 8.7 | 0.4 | 15 | |||
Notes. Column 1: Source name; Column 2: mJIVE-20 identifier; Column 3: optical identification: G = galaxy; Q = quasar; E = empty field in optical images; s = stellar object. Column 4: optical r-band ab magnitude from the DESI Legacy Surveys. A * indicates z-band magnitude; Column 5: photometric redshift from DESI Legacy Surveys Data Release 9 (Zhou et al. 2023). An sp denotes a spectroscopic redshift from SDSS data; Column 6: W1-band (3.4μm) VEGA magnitude from WISE; Column 7: VLBI peak flux density (mJy beam−1); Columns 8 and 9: total flux density (mJy), at 1.4 GHz from FIRST and 3.0 GHz from VLASS data, respectively; Column 10: spectral index between 1.4 GHz (from FIRST data) and 3.0 GHz (from VLASS); Column 11: largest angular scale. The sources discussed in this paper are marked in bold.
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