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Fig. 2

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Upper panel: decomposition of the quasar spectrum into a macrolensed-only component (FM, black line) and a component both macro- and microlensed (F, blue line) by applying MmD to the spectra of images B and D. F is shifted upward by three units. The spectrum of image B (FB, grey line), assumed to be unaltered by microlensing, is shifted downward till its continuum intensity is null and is superimposed on FM. The spectra are filtered with a five-pixel-wide median filter for clarity. The vertical dotted line indicates the redshifted rest wavelength of the Hα line. Lower panel: same for the pair of spectra of images B and A.

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