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Fig. 1.

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Flowchart of the matching processes and sample selections (see details in Sect. 2). (1)Details about broadband SED fitting can be found in Sect. 3.1 and Appendix A. (2)Details about IR-radio correlation (IRRC) analysis can be found in Sect. 4. (3)Details about the radio luminosity function can be found in Sect. 5. (4)Details about the maximum-likelihood (ML) fitting method used for calculating the probability of hosting a radio-excess AGN can be found in Sect. 6. (*)LTIR: rest-frame total IR luminosity between 8 and 1000 μm.

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