Notes. Col. (1): Instrument considered. The references L15, L18, and L23 correspond to Longinotti et al. (2015), Longinotti et al. (2018), and Longinotti et al. (2023), which report the derivation of the outflow parameters based on XMM-Newton, LMT, and NOEMA data, respectively. The original and scaled results from these datasets are also shown. In boldface we highlight the main MEGARA results derived under our assumptions (see text). The star symbol (^★) marks the NOEMA and MEGARA results that can be directly compared, since they used the same v_out formula (see Col. 9). The NOEMA values were normalized using C = 1 (see text for details). Col (2): velocity of the outflow derived according to the formula described in Col (9). Col (3-7): mass of the outflow, mass outflow rate, kinetic energy of the outflow and kinetic power of the outflow obtained following Eqs. (5), (6), (7) (see text for details). The molecular radius derived in Longinotti et al. (2023) is R_CO = 2.8 ± 0.3 kpc. The intrinsic ionized outflow radius derived in this work is R_out(Hα) = 0.98 ± 0.32 kpc. Col (8): ratio between the momentum rate of the outflow Ṗ_out and Ṗ_rad = L_bol/c = 1.7 × 10³⁴ g cm s⁻² is the radiation force of the AGN, with L_bol = 5.2 × 10⁴⁴ erg s⁻¹ (Giroletti et al. 2017; Longinotti et al. 2018). Col (9): Assumptions considered to derive the outflow parameters with the different instruments: (i) to derive the ionized outflow velocity, two formulas are used: v_out = Δv + 1.18 σ_B from Rupke et al. (2005) (RV05), and v_out = Δv + 2 σ_B from Rupke & Veilleux (2013) (RV13); (ii) to derive the ionized outflow mass, two electron densities (n_e = 500 and 2500 cm⁻³) are considered for the MEGARA data; (iii) to derive the molecular outflow mass, two CO-to-H2 conversion factor values, α_CO, are considered in Longinotti et al. (2023): α_CO = 0.5 and 0.8 M_⊙ (K km s⁻¹ pc²)⁻¹.