Notes. The A_V values were measured using H_α/H_β reported by Kong & Ho (2018), and the extinction law is from Cardelli et al. (1989). The only exception is J1356, whose A_V value is unrealistically low (0.1 mag), and therefore we use the value measured from VLT/MUSE data instead, as in Zanchettin et al. (2025). Bolometric luminosities were calculated by applying the correction factor of 474 from Lamastra et al. (2009) to the extinction-corrected [O III]5007 Å luminosities from Kong & Ho (2018), and 1.4 GHz luminosities and stellar masses are from Ramos Almeida et al. (2022). The BH masses and Eddington ratios are from Kong & Ho (2018). The last two columns are the global SFRs derived from total IR luminosities from Ramos Almeida et al. (2022), divided by 0.94 to convert them from a Chabrier to a Kroupa initial mass function, and the SFRs were derived by Bessiere et al. (2024) from spectral synthesis modeling of the SDSS spectra (3″ ∼ 5–6 kpc) shown in Fig. A.1..