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Fig. 4


Examples of our low-resolution dereddened spectra (magenta lines) and their model SEDs (black lines) at selected dates prior to and during the 2015 outburst of AG Peg. Denotation of lines is as in Fig. 3. Contribution from the WD corresponds to parameters in Table 5. It is negligibly small throughout the optical. Modelling is described in Sect. 3.2.1.

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