Table 2.
Dominant radio mechanism indicators and overall source classification.
| Object | L1.4 GHz | VLASS variability | Radio spectra | Radio morphology | FIR-radio correlation |  |
Rk | Overall Classification |
|---|---|---|---|---|---|---|---|---|
| J00418+4021 | – | – | Linear/Curved | Extended | SF | SF | RL | SF dominated |
| J00457+0410 | – | – | – | – | – | – | – | – |
| J00535+1241 | – | – | Linear/Curved | C/I | SF | SF | RQ | SF dominated |
| J10255+5140 | – | – | Linear/Curved | C/I | SF | SF | RQ | SF dominated |
| J11292-0424 | – | – | Linear/Curved | C/I | SF | SF | RQ | SF dominated |
| J11420+6030 | – | – | Linear/Curved | C/I | – | Combination | RQ | Core/Jet + SF |
| J12075+1506 | Core/Jet | – | Linear/Curved | C/I | – | SF | RQ | Core/Jet + SF |
| J12091+5611 | – | Core/Jet | Linear/Curved | C/I | – | Core/Jet | RL | Core/Jet dominated |
| J12366+5630 | – | – | Linear/Curved | C/I | – | Combination | RL | Core/Jet + SF |
| J12562+5652 | – | Core/Jet | Flat/Inverted | Extended | SF | SF | RL | Core/Jet + SF |
| J13012+5902 | – | – | – | – | – | – | – | – |
| J14052+2555 | – | – | Linear/Curved | C/I | SF | SF | RQ | SF dominated |
| J14063+2223 | – | – | Linear/Curved | C/I | – | SF | RQ | SF dominated |
| J14170+4456 | – | – | Linear/Curved | C/I | SF | SF | RQ | SF dominated |
| J14258+3946 | Core/Jet | – | Flat/Inverted | C/I | – | Core/Jet | RL | Core/jet dominated |
| J14475+3455 | Core/Jet | - | Linear/Curved | C/I | SF | Combination | RL | Core/Jet + SF |
| J15455+4846 | – | Core/Jet | Linear/Curved | C/I | SF | SF | RL | Core/Jet + SF |
| J17014+5149 | Core/Jet | – | Linear/Curved | Jets | SF | Combination | RL | Jet dominated |
Notes. Column 1: Object coordinate name. Column 2: Sources with log L1.4 GHz > 31.6 erg s−1 Hz−1 likely have an AGN-related contribution to their radio emission. Column 3: Variability index V > 0.1 (based on VLASS) indicate core or jet origin. Column 4: Shape of the radio spectrum. Column 5: Radio morphology: extended, compact, intermediate (C/I), or presence of jets. Column 6: Sources for which pSFRradio ≃ SFR60 μm are likely SF-dominated; sources below the correlation are likely a combination. Column 7: Sources with 
are SF; those with 
are core or jet-dominated and the remainder are a combination. Column 8: Kellermann’s parameter Rk (same as in the last column of Table B.2). Column 9: Overall origin of the emission mechanism.
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