Notes. In the best-fit models the iron K emission and absorption lines, with their Gaussians model parameters are included and reported separately in Table 2. The 𝒩ℋℳ used in Sect. 4.4 consist of the best-fitting models reported here minus the Gaussian absorption components. Flux in the 4–10 keV band in units of (erg cm⁻² s⁻¹). Reduced 𝒞stat and number of degrees of freedom (ν) for the final best-fit model. All the WA components are required at P_F > 99%. 𝒞−stat using the number of bins (ζ) in each EPIC detector and the total 𝒞−stat with the degree of freedoms (ν) corresponding to the final best-fit model. ⊞ A narrow (10 eV) Gaussian absorption line of rest-frame energy of E = 3.51 ± 0.06 keV was required at 3σ (99.7%) confidence level. † Seyfert 2 target with an intrinsic neutral absorber with column density of . The soft X-ray band < 2 keV was modelled with two thermal emission components with apec yielding eV, and eV, with normalisations in unit of where D_A is the angular diameter distance to the source in cm, n_e and n_H are the electron and H densities (cm⁻³), respectively. A narrow/strong Gaussian emission line of E = 2.35 ± 0.04 keV was required at 3.6σ (> 99.9%) confidence level. ^‡ Intrinsic neutral absorber with required at P_F > 99.99% and two narrow soft X-ray emission at keV and keV both at P_F > 99.99%.