Notes. Col. (1) the source name; Col. (2) the other name; Col. (3) redshift; Cols. (4) and (5) classification [low-excitation or high-excitation radio galaxies (LERGs or HERGs)] and its reference; Col. (6) γ-ray photon index; Col.(7) γ-ray luminosities in the unit of erg/s; Cols. (8) and (9) the CD and its reference; Cols. (10) and (11) the bolometric luminosity and its reference; Cols. (12) and (13) the accretion rate and its reference. If the stellar velocity dispersions from the SDSS and/or HyperLeda website (http://atlas.obs-hp.fr/hyperleda, Makarov et al. 2014) are available, then the BH masses are computed from the relation between the BH masses and velocity dispersion (Tremaine et al. 2002) (S-T02 or M14-T02); otherwise, the BH masses are obtained from the literature. References: S72 for Shields et al. (1972), G83 for Grandi (1983), B89 for de Bruyn (1989), B92 for Baum et al. (1992), H97 for Ho et al. (1997), H99 for Ho (1999), W00 for Werner et al. (2000), K03 for Kim & Fabbiano (2003), B09 for Buttiglione et al. (2009), J09 for Jones et al. (2009), E10 for Evans et al. (2010), I10 for Inskip et al. (2010), S14 for for Sadler et al. (2014), MI14 for Mingo et al. (2014), B16 for van den Bosch (2016), J16 for Janiak et al. (2016), B18 for Bassi et al. (2018), H20 for Hlabathe et al. (2020), B21 for Balasubramaniam et al. (2021), P21 for Paliya et al. (2021); C23 for Chen et al. (2023), P23 for Pannikkote et al. (2023). SDSS for Sloan Digital Sky Survey (www.sdss.org, Abdurro’uf et al. 2022).