Best-fit spectrum of 1H 0707–495 in E * F(E) units during: (a) LHS using Suzaku observation 00091623; (b) (IS) using Swift observation 00091623002; (c) IS using ASCA observation 73043000; and (d) HSS using Swift observation 00080720048. The data are presented by crosses and the best-fit spectral model tbabs*(BMC+N*Laor) by red line. The Comptonization hump component is shown by the dotted sea-green line. To model the Laor line components, we used the N XVII (blue), O III (green), Fe XVII (bright blue), Ne X (pink), S XVI (orange), Fe I–XXII, and Fe XXV/Fe XXVI K_α (yellow) lines with energies of 0.5, 0.65, 0.85, 1.02, 2.9, 6.4, and 6.8 keV, respectively. Bottom: Δχ vs photon energy in keV.