Fig. 1
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SEDs of two white dwarfs (Gaia DR3 1900545847646195840 and Gaia DR3 5187830356195791488) showing IR excess emission. The left-hand panel shows an example of a DA model fit, and the right-hand panel an example of a non-DA model fit. Models are shown with blue lines and the photometric data with black or red points depending on whether excess flux emission with respect to the model is detected or not, respectively.
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