Notes. Columns from left to right report: the system name; redshift; classification (GG: Galaxy Group, MMC: Massive Merging Cluster, MRC: Massive Relaxed Cluster, LMC: Low-mass Merging Cluster, LRC: Low-mass Relaxed Cluster); the assumed density model (β for a single β-model, 2β for a sum of two β-models, dβ for a sum in quadrature, and univ. for the universal profile introduced by Ghirardini et al. 2019); central thermal density n₀; core radius r_c; and the β index. Additional parameters are provided in the subsequent row where necessary; specifically, for the universal model, the second n₀, β, and r_c values correspond to α, ϵ, and R_s, respectively. The table also lists: the magnetic field power spectrum model (’pl’ for power law, ’bpl’ for broken power law, and ’df’ for the model proposed by Domínguez-Fernández et al. 2019); the spectral slope ζ; and the Λ_min and Λ_max scales. For the ’df’ profile, ζ and the second Λ_min correspond to parameters B and C, respectively. Radial profile parameters for the magnetic field (B₀ and η) are also included. We note that 3C449 is the only case with a broken profile, characterized by η = 0 at radial distances exceeding 16 kpc. Finally, we report the mass and radius computed within R₅₀₀ (Piffaretti et al. 2011). Parameters assumed a priori in the original modelling are highlighted with an asterisk. All spatial scales, densities, and magnetic field strengths have been rescaled to the cosmology adopted in this work. For 3C31 and Hydra A, we rescaled the reported B_rms values according to B_rms = 0.42B₀ (Laing et al. 2008). For A2255, we refer to the modelling based on radio galaxy RMs (Govoni et al. 2006). In the case of 3C31, we used results obtained without cavity modelling, as these features were not detected. For both A2345 and A2142, B₀ was extrapolated from the average magnetic field strength within a 1 Mpc³ volume reported by the authors, assuming the radial profile parameters (η, n_e) derived for the system. Central temperatures for A665 and A523 were taken from Norseth et al. (2025) and Cova et al. (2019), respectively. Literature data are sourced from: Guidetti et al. (2010) (3C449), Laing et al. (2008) (3C31, Hydra A), Murgia et al. (2004) (A119), Govoni et al. (2017) (A194),Pagliotta et al. (2025) (A2142), Vacca et al. (2012) (A2199), Govoni et al. (2006) (A2255), Stuardi et al. (2021) (A2345), Guidetti et al. (2008) (A2382), Vogt & Enßlin (2003) (A2634 and A400), Khadir et al. (2026) (A3581), Vacca et al. (2022) (A523), Vacca et al. (2010) (A665), Bonafede et al. (2010) (Coma Cluster), and this work (Fornax cluster).