The q_TIR parameter over redshift for the sample explored by Enia et al. (2022) and for our 8 galaxies (panel a). This figure was retrieved by Enia et al. (2022), published under the CC BY 4.0 international licence and was modified by adding the results from our work (square points). The dashed black line and grey shaded region correspond to the best-fit relation of their total sample and the standard deviation, respectively, while the dashed blue line shows a similar relation by Delhaize et al. (2017). All points by Enia et al. (2022) are coloured according to the contribution of AGN to the radio emission defined as , with q_tot and corresponding to the q_TIR and its evolution with redshift, respectively. The star symbols depict what is defined by Enia et al. (2022) as H-dark sources (i.e., not detected at the Hubble-WFC3 H-band). Panel b, presents the SFRs derived from the IR and radio luminosity, for the 8 sources of our sample, along with the results by Bonzini et al. (2015) (radio-quiet AGN: blue squares, radio-loud AGN: red triangles, SF galaxies: green circles) and Talia et al. (2021) (average values of their sample). All data points with redshift below 3 are coloured with transparency, while the ones with z > 3 have normal colours.